The galaxy appears as a slightly elongated, lenticular-like structure. The central bulge is bright and concentrated, exhibiting a yellowish-white hue, which likely indicates an older stellar population dominating this region. Extending outwards from the bulge is a fainter, bluer disk-like component. The disk appears relatively smooth, without prominent spiral arm structures visible in this image. The smooth appearance suggests either a lack of significant ongoing star formation or a viewing angle that obscures spiral features. There is a slight asymmetry to the galaxy's shape, with one side appearing somewhat more extended or diffuse than the other, although there does not appear to be any major merger event occurring. The galaxy seems to be relatively isolated, not displaying strong tidal interactions with nearby galaxies. Overall, the galaxy presents an elliptical shape with a hint of disk-like structure, possibly an edge-on spiral or lenticular galaxy.
