This galaxy presents as a relatively smooth, elliptical object with an approximate effective radius of 4.6 kpc. The central region exhibits a concentrated, bright core. The color profile suggests a population of older stars dominating the light output, with a slight reddening from the center outwards. There is a lack of distinct spiral arm structures or prominent dust lanes, indicating a probable evolved system with little ongoing star formation. The overall shape tends more toward an in-between roundness than a flattened disk, supporting the elliptical classification. There is no obvious evidence of recent or ongoing major mergers; the galaxy appears largely undisturbed, potentially having experienced minor gravitational disturbances in the past.
