The galaxy presents as a centrally concentrated object, exhibiting a relatively smooth morphology. The central region displays a bright, yellowish hue, suggestive of an older stellar population. Moving outwards from the center, the color transitions subtly to a bluer tint in the outer regions, indicative of younger stars. The overall shape is approximately round, with minimal signs of spiral arms or significant disk structure. There appear to be no prominent tidal features or distortions, suggesting a lack of recent major merger events. The galaxy exhibits a slight elongation.
