The galaxy presents as a relatively smooth, elliptical-like structure, with a bright central bulge. The color profile is centrally concentrated, appearing yellow-white in the core, suggesting an older stellar population. Moving outward from the center, the light fades gradually with a slight shift towards redder hues, although no distinct spiral arm features or prominent dust lanes are visible. There are hints of some minor disturbance or possible merging event. The outer regions of the galaxy appear amorphous and indistinct, lacking sharp boundaries, suggesting a gradual transition into the intergalactic medium. The overall morphology points towards a system that has largely completed its major star formation phase, with any ongoing star formation likely occurring at a lower rate.
