The galaxy presents a largely smooth and centrally concentrated light distribution, indicative of an elliptical or lenticular morphology. The galaxy's core is notably bright, exhibiting a yellowish-white hue. The outer regions appear fainter, transitioning to a slightly more reddish tone. The overall shape is generally round, with only subtle deviations from perfect circularity. There is no obvious spiral arm structure or significant dust lane obscuration visible. Faint indications of minor disturbances, such as slight tidal tails or asymmetries, are not entirely ruled out but are not prominently featured. There is a hint of what appears to be a subtle and unresolved tidal feature in the upper region of the galaxy. Based on the observed color gradient, there may be a difference in the stellar populations between the core and outer regions, with the core potentially hosting older stars, and more recent star formation occurring in the outer parts.
