The galaxy presents as a largely smooth, elliptical structure with a concentrated central bulge. There is minimal evidence of spiral arm features or significant dust lanes. The color profile indicates a population of older stars, with a yellowish hue dominating the central region. The galaxy appears relatively isolated, with no immediately obvious signs of ongoing major merging activity or tidal distortions, though there is a slight asymmetry in the shape, perhaps indicating a minor disturbance. The galaxy is somewhat elongated with a moderate ellipticity. The overall appearance suggests a mature galaxy with a relatively low star formation rate.
