The galaxy presents as a relatively compact structure with a discernible, albeit somewhat disturbed, morphology. The object's overall form appears nearly circular in projection. The light distribution suggests a centrally concentrated luminosity profile, hinting at a dominant bulge component, although there appears to be a slight elongation or asymmetry in the outskirts, possibly indicative of minor tidal interactions or ongoing disturbances.

The galaxy exhibits a color gradient. The central region shows a yellow-red hue. Moving outward, there are blue-green tinges. This suggests a transition from an older stellar population in the center to regions with more recent star formation activity in the outer regions.

There is a distinct lack of well-defined spiral arms, indicating either a primarily spheroidal structure or a disrupted spiral morphology. Patches of brighter regions are visible, possibly due to active star-forming regions. Overall, the galaxy presents as a system that may be in a state of transition, either through internal processes or external interactions, leading to its observed disturbed morphology and mixed stellar populations.
