The galaxy presents as a somewhat elongated, lenticular system. It exhibits a bright, concentrated central bulge, possibly indicative of an older stellar population. The bulge gradually transitions into a fainter, disk-like structure that extends along the major axis. The disk appears relatively smooth with only faint hints of spiral arm structure, suggesting a relatively quiescent star formation rate. The overall color is biased towards the redder end of the spectrum, supporting the inference of an older stellar population. There is no visually significant dust lane obscuring the central bulge and only very slight asymmetry. The smooth, elongated shape indicates that the galaxy is likely an elliptical- or lenticular-type, seen from a considerable angle. No major signs of tidal disturbances or interactions with neighbor galaxies were observed.
