The galaxy presents as a centrally concentrated, elliptical or lenticular system. It exhibits a smooth, diffuse luminosity profile with no apparent spiral arm structures or prominent dust lanes. The core region is bright, suggesting a high density of stars. The overall shape is moderately elongated, neither perfectly spherical nor highly flattened, with a suggestion of a cigar shape. There are no obvious signs of ongoing major mergers or significant tidal disturbances, though very subtle minor disturbances cannot be ruled out. The color index suggests a population of older stars, which is consistent with the smooth morphology. There is faint blueish hinting at the presence of hot, young stars, though star formation is likely suppressed. The galaxy appears relatively isolated in the field of view. Based on its morphology and color, it is likely to be a relatively massive system.
