This galaxy exhibits an elliptical morphology, appearing largely smooth and spheroidal. Its color profile suggests a population of older stars, with a yellowish-red hue dominating. The light is centrally concentrated, with brightness decreasing gradually from the core outwards. There is no visible disk structure or spiral arm features. The galaxy does not show any major signs of tidal disturbances or recent merger activity. Faint, extended light may be present in the outer regions, but is not a distinct feature. Based on its color and morphology, the galaxy likely has a relatively low star formation rate. It appears to be a relatively massive system.
