The galaxy presents as a singular, somewhat elliptical, and largely smooth structure. There is a brighter, condensed central region, possibly indicative of a galactic nucleus. The overall color of the galaxy appears yellowish-orange, suggesting a population of older stars and a relatively low rate of ongoing star formation. The galaxy exhibits some evidence of tidal disruption. A secondary object nearby is a likely component in this disturbance. There may be ongoing or recent merger activity. The structure is fairly rounded.
