The galaxy presents as a relatively smooth, rounded object. It appears to be fairly compact in size, exhibiting a predominantly elliptical morphology. The galaxy displays a noticeable color gradient, transitioning from a slightly bluer hue in its central regions to a redder tone in its outer regions. This color variation might be indicative of differing stellar populations, with younger, bluer stars concentrated towards the center and older, redder stars dominating the outskirts. There is no strong evidence of spiral arm structure or significant dust lanes. There are potentially minor disturbances or asymmetries visible, though not particularly prominent. It is potentially undergoing a minor interaction or exhibiting internal irregularities.
