The galaxy appears to be a relatively massive, elliptical galaxy at a redshift of approximately 0.3. It exhibits a smooth, centralized light distribution, with the majority of its light concentrated in a centrally located bulge. The galaxy is elongated in shape, displaying a notable axis ratio. Its color index indicates a population of older stars, characterized by redder hues. No strong evidence of active star formation regions, spiral arms, or significant dust lanes are immediately visible. The overall morphology is consistent with an early-type galaxy. There is a possible minor disturbance present, however it doesn't seem to be undergoing a major merger event.
