The galaxy presents as an elliptical morphology with a smooth, concentrated central bulge. The light distribution is centrally concentrated with a high Sersic index, indicating a steep decline in surface brightness away from the core. The color profile suggests a relatively old stellar population, given the redder hue observed. There is a slight asymmetry, potentially due to a minor interaction or internal dust lanes, but it appears to be a largely undisturbed system. The overall structure suggests a mature galaxy with little ongoing star formation.
