The galaxy presents as a moderately luminous, fairly compact object, approximately 7 kiloparsecs in effective radius. The overall morphology appears relatively smooth, with a dominant elliptical-like profile. There are minimal visible features suggesting spiral arms or prominent dust lanes. Color gradients show a tendency towards redder hues in the central region, indicative of older stellar populations. The outer regions exhibit somewhat bluer colors, potentially suggesting ongoing, albeit subdued, star formation. There is no obvious evidence of a major merger event or significant tidal disturbance. The structure is moderately elliptical in shape, appearing somewhat elongated rather than perfectly circular. Marginal evidence of minor disturbances cannot be excluded given the limited image resolution.
