The galaxy presents as a flattened, elliptical morphology. Its light profile appears relatively smooth and centrally concentrated, lacking prominent spiral arms or significant irregular features. The overall color is fairly homogenous, with a central region displaying a slightly bluer hue compared to the outer regions, which exhibit a redder color profile. The blue core possibly indicates more recent, ongoing star formation in the inner region. The galaxy appears to have a well-defined edge, gradually fading into the background. There is no evidence of strong tidal interactions or ongoing mergers that would significantly disrupt its overall shape. The galaxy has a small amount of neutral hydrogen.
