The galaxy presents a moderately elliptical morphology, appearing somewhat smoothed and diffuse. A discernible central bulge region exhibits a yellowish hue, suggestive of an older stellar population. The outer regions of the galaxy display a bluer color, possibly indicating ongoing, albeit subdued, star formation activity. Evidence suggests that the galaxy has undergone minor disturbance, although a merger event does not appear to be the predominant explanation. There is no obvious presence of spiral arms or a well-defined disk structure. It appears relatively isolated, without any obvious, large companions, although there are indications of faint streams or tidal features, possibly from past interactions.
