The galaxy appears as a slightly elongated, lenticular-like system with a smooth, diffuse structure. The central region exhibits a bright, concentrated bulge that gradually fades into the outer regions. The color profile shows a subtle gradient, with the core appearing more yellow, possibly indicating an older stellar population. The outer disk exhibits bluer hues, suggesting the presence of younger, hotter stars, although their contribution seems minimal. There is a lack of distinct spiral arm structure. The morphology is broadly consistent with an early-type spiral or lenticular galaxy, possessing a notable spheroidal component and a relatively quiescent star formation rate. The overall appearance suggests a galaxy that has largely ceased active star formation within its central regions. The isophotes are moderately elongated, deviating noticeably from a perfectly circular shape. There's a minor asymmetry in the brightness distribution along the galaxy's major axis.
