The galaxy presents as a relatively compact object with a moderately bright core. It exhibits a somewhat elliptical morphology, appearing largely smooth in its overall structure. Evidence suggests the presence of some internal features, potentially indicative of a faint disk or spiral arms, although these are not sharply defined. The galaxy displays a color gradient, with the central regions showing a more yellow/red hue compared to the outer edges, which appear slightly bluer. This color variation could suggest differences in stellar populations, with older, redder stars concentrated towards the center and younger, bluer stars populating the outskirts. There is a suggestion of minor disturbances to the structure, and these faint tidal tails hint at past or ongoing minor interactions with other galaxies, although no clear signs of a major merger event are immediately apparent in this image.
