The galaxy presents as a single, largely featureless object with a smooth, elliptical morphology. Its color is predominantly yellowish-orange, suggesting a population of older stars and a relatively low rate of on-going star formation. There is no evidence of spiral arms or a distinct disk structure. The galaxy appears highly symmetrical, with no noticeable tidal tails, asymmetries, or other indications of recent or ongoing merger activity. The light distribution is concentrated towards the center, gradually diminishing outwards. The rounded appearance indicates a classification leaning towards an E0-E3 on the Hubble Sequence. The galaxy is at an estimated distance corresponding to a redshift of approximately z = 0.24.
