The observed galaxy presents a complex morphology, appearing neither purely elliptical nor a well-defined spiral. There is evidence of both smooth, centrally concentrated light as well as more diffuse, extended features. The galaxy exhibits a prominent central bulge, which appears to be roughly circular and yellow-orange in color. This suggests an older stellar population dominating the core.

Surrounding this central region, fainter and more diffuse material is visible, exhibiting a slightly bluer hue. This suggests the presence of younger stars or regions of active star formation outside of the bulge. The distribution of this bluer material is somewhat irregular and lumpy, indicating possible interactions with another galaxy. There may be some tidal tails or other features indicating a past or ongoing gravitational disturbance.
