The galaxy presents as a relatively smooth, elliptical structure. Its color profile is dominated by reddish-yellow hues, suggesting a population of older stars with relatively low ongoing star formation. The light is concentrated towards the center with a gradual falloff towards the edges. The galaxy has an elongated shape, but is neither extremely flattened nor cigar-shaped. There is no apparent evidence of major mergers or significant tidal disturbances. The galaxy appears to be relatively isolated.
