The galaxy appears to be a lenticular or early-type spiral, exhibiting a smooth, elliptical morphology. It is observed nearly edge-on, with a distinct major axis longer than its minor axis. The central bulge is prominent and exhibits a concentration of light, suggesting a high stellar density. The bulge appears reddish, possibly indicating an older stellar population. Fainter, bluer light is distributed throughout the disk surrounding the bulge, perhaps due to the presence of some younger stars. There is no clear evidence of spiral arm structure, and the galaxy appears relatively undisturbed, without signs of ongoing major mergers or tidal interactions. Some minor disturbances may be indicated by the asymmetric light distribution.
