The galaxy appears as a relatively smooth, elliptical structure with a concentrated central bulge. The light distribution is quite even, indicating a lack of significant star-forming regions. Its color profile suggests an older stellar population, with a yellowish-red hue dominating, which is typical of early-type galaxies. The roundness is fairly pronounced, though there is a slight elongation visible. There is no evident presence of tidal tails, rings, or other features indicative of recent or ongoing major mergers. Light deviations suggest there is a chance the galaxy is undergoing a minor merger.
