This galaxy appears to be a relatively compact object. Its light is somewhat smooth and centrally concentrated, suggesting an elliptical morphology, but there appears to be a slightly elongated shape. There is no obvious presence of spiral arms, bars, or significant dust lanes. The galaxy exhibits a slight color gradient, becoming slightly redder towards the center, which could indicate a population of older stars in the galactic core. There are no signs of any ongoing major mergers or violent starburst activity, however there appears to be some slight disturbances in the surrounding galactic halo that could indicate minor disturbances or past minor mergers. The galaxy seems to be a significant distance away, due to its redshift and apparent size.
