The galaxy appears as a concentrated, centrally brightened object with an overall smooth morphology. There is a slight elongation, but it is mostly rounded in shape. It exhibits a predominantly yellow/orange hue, indicative of an older stellar population. There is no obvious spiral structure or prominent dust lanes visible. Slight asymmetry or minor disturbances in the outer regions might be present, although the resolution makes this hard to identify definitively. There is no apparent major merger activity or strong tidal features.
