The galaxy presents as a relatively smooth, centrally concentrated object with a roughly elliptical morphology. There is a slight elongation visible, but the overall structure appears to be dominated by a spheroidal component. The color profile suggests a population of older stars, contributing to its reddish hue. A weak tidal tail or plume extends from the main body of the galaxy, which suggests some interaction in the past. Some faint knots of bluer material could be the result of on going star formation. There is no obvious central bulge, however, the core appears to be denser than its surrounding areas. The image does not reveal any prominent spiral arm structures, but its classification is uncertain without further spectral analysis.
