The galaxy presents as a largely elliptical or spheroidal structure. It is relatively smooth in appearance, with minimal evidence of spiral arms or a distinct disk. There is a slight elongation, though the overall shape is predominantly round. There are no signs of a major ongoing merger or significant tidal disturbances. The galaxy exhibits a redder hue in the color composite image, which may indicate a population dominated by older stars and a relatively low rate of ongoing star formation. There are some hints of low-level disturbances, such as a slight asymmetry in the light distribution. The galaxy possesses a concentrated central region surrounded by a more diffuse halo of stars.
