This galaxy appears to be a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge. It displays a yellowish hue, suggesting a stellar population dominated by older stars. The overall shape is largely spheroidal, with a lack of apparent spiral arm structure or significant dust lanes. There is no obvious signs of any major merger events or interactions affecting the galaxy's morphology, although there may be a minor disturbance to the smoothness of the light profile. It is considered generally isolated, with a moderate mass and a relatively low star formation rate.
