The galaxy presents as a lenticular or possibly an elliptical galaxy, exhibiting a relatively smooth, diffuse light distribution with a prominent bulge. The central region displays a high concentration of light, gradually diminishing towards the outer edges.

There is a suggestion of a faint disk structure, though ill-defined and viewed at a shallow angle. The galaxy shows a generally homogenous color profile, with a tendency towards yellow or orange hues in the central region, potentially indicating an older stellar population. The outer regions have a slight bluer tinge.

There are no discernible spiral arms or prominent dust lanes. The overall morphology suggests a relatively evolved system, possibly undergoing or having completed the process of transitioning from a spiral to a more quiescent elliptical or lenticular form. There is a possible distortion to the shape of the overall system. There does not appear to be a substantial amount of ongoing star formation.
