The galaxy presents as a relatively compact, elliptical-like structure with a smooth, featureless appearance. Its light distribution appears centrally concentrated, lacking any significant spiral arm structures or prominent dust lanes. The color profile suggests a dominant population of older stars, giving it a yellowish-red hue. The overall morphology indicates a system that is highly spherical, with little indication of tidal disturbances or recent merger events. There is no evidence of a bright, actively star-forming nucleus, suggesting a low rate of current star formation.
