The galaxy presents as a primarily smooth object with a slight elongation, appearing more akin to a lenticular or early-type spiral galaxy viewed at an angle. The light distribution indicates a concentrated central bulge, with a fainter, diffuse disk extending outwards. There is a subtle hint of a spiral structure but it is not well-defined. The overall color is relatively uniform, suggestive of an older stellar population with limited ongoing star formation. There are subtle variations in color across the galaxy, with some regions appearing slightly bluer, possibly indicating areas of recent, albeit subdued, star formation. There is no evidence of significant tidal disturbances or ongoing mergers, suggesting it is a relatively isolated system currently undergoing quiescent evolution.
