The galaxy presents as an elliptical or lenticular type, exhibiting a relatively smooth light distribution without prominent spiral arms or a distinct disk structure. The central bulge region appears bright and concentrated, suggesting a high stellar density. Moving outwards, the galaxy fades gradually into the surrounding space, with a diffuse halo that lacks sharp boundaries.

There is a slight elongation in the galaxy's shape, deviating from a perfect circular form. A subtle color gradient is observed, with the central regions exhibiting a yellowish or golden hue, possibly indicating an older stellar population. The outer regions seem to have a bluer tinge, which may be caused by some younger stars.

There may be a slight distortion or minor interaction visible, with subtle irregularities in the light distribution on one side, suggesting potential past interactions. However, the overall structure appears to be relatively undisturbed, without significant tidal tails or signs of a major ongoing merger. The galaxy does not show any obvious dust lanes or prominent star-forming regions.
