The galaxy appears as a centrally concentrated, elliptical or lenticular system. It exhibits a smooth luminosity profile, with the brightest region located at the core, gradually decreasing in intensity outwards. The central region displays a yellowish-white hue, suggesting a population of older stars and a relative lack of ongoing star formation. Fainter, bluish-toned regions extend around the core, indicating some presence of younger, hotter stars, which may be located in a possible disk or faint spiral structure. The galaxy is fairly round in appearance, with only a slight deviation from perfect circularity. There is no strong evidence of any ongoing major merger events or tidal disturbances.
