The galaxy presents an overall smooth appearance, with a slight elongation suggesting a shape that is somewhere between round and cigar-shaped. While it does not exhibit a classical spiral structure, there is a subtle hint of a disk-like component. The light distribution is centrally concentrated, fading smoothly outwards from the core. There may be some minor disturbances, possibly indicative of a weak tidal interaction or past merger event. The galaxy's color appears to be moderately red, suggestive of a population of older stars and a relatively low current star formation rate.
