The galaxy presents a smooth, elliptical morphology. It appears predominantly featureless, with a concentrated central bulge that gradually fades into the outer regions. The color gradient suggests a population of older stars, contributing to a yellow-red hue in the core region. A slight bluer tint is seen in the outer areas, suggestive of younger star formation regions in the disk. There are no apparent spiral arm structures or significant dust lanes visible. The overall shape appears close to round, with a high degree of symmetry. There is no evidence of any ongoing merger activity, or of any significant tidal disturbances. The galaxy displays a fairly concentrated light profile. The galaxy measures an estimated diameter of approximately 7 kpc.
