The galaxy appears as a roughly circular, relatively smooth object. A concentrated central bulge is clearly visible, surrounded by a fainter, more diffuse halo. The light distribution is fairly uniform without strong spiral arm structures or prominent dust lanes. The galaxy exhibits a color gradient, with the central region appearing slightly redder compared to the outer regions, which have a bluer hue. This color difference may suggest variations in stellar populations, with older, redder stars dominating the center and younger, bluer stars being more prevalent in the outer disk. There are subtle hints of asymmetry in the outer regions, but it's difficult to determine if this is due to interactions or intrinsic features. The galaxy does not appear to be undergoing any major merging events, although there is the possibility of a minor disturbance or a past interaction that has since settled. Overall, this galaxy seems to be a relatively quiescent system, likely an elliptical or lenticular galaxy at moderate redshift.
