The galaxy presents a primarily smooth morphology, with a noticeable central bulge. The galaxy exhibits a generally elliptical shape but appears slightly elongated. The color profile suggests an older stellar population, likely dominated by redder stars with some regions of bluer, potentially younger stars mixed within, indicating ongoing or recent star formation. There is evidence of some minor disturbance, possibly from a small gravitational interaction, but appears generally settled with some irregularities. The overall structure does not suggest a major ongoing merger. It exhibits a compact size, with a concentrated luminosity profile.
