The galaxy presents as a centrally concentrated, elliptical-like object. The light distribution appears smooth and generally featureless. There is little evidence of spiral arms, bars, or prominent dust lanes. The color profile suggests a more evolved stellar population, leaning towards yellow and red wavelengths, with a faint greenish hue. The overall morphology indicates a system that has likely undergone significant dynamical relaxation, approaching a spheroidal shape. There is no obvious evidence of a recent major merger or significant tidal interaction. The galaxy exhibits a concentrated form, with a clear peak in luminosity towards the center.
