The galaxy presents a primarily smooth morphology, with a significant fraction of its light concentrated in a central bulge. The bulge appears approximately round. A faint disk-like structure is potentially present, although its contribution to the overall light profile is minor. There is a possible minor disturbance in the system, perhaps a small tidal feature or companion galaxy interacting with the primary galaxy. There may also be a slight hint of ongoing star formation in the outer regions. The light from the bulge shows a color gradient suggestive of an older stellar population. The galaxy appears to be a reasonably massive system.
