The galaxy presents a largely smooth, elliptical morphology. It exhibits a centrally concentrated luminosity profile, fading outwards with no discernible spiral arms or bar structure. The galaxy appears to be relatively isolated with no nearby companions showing signs of significant tidal distortion. There is some evidence of a slight elongation in the shape, but not markedly cigar-shaped. The color indices suggest a population dominated by older stars. The galaxy has a measurable amount of star formation.
