This galaxy appears to be an elliptical or lenticular galaxy at a significant redshift. The light profile is smooth, with a highly concentrated central region, suggesting an older stellar population. The overall shape is relatively round. There are no signs of spiral arms or prominent dust lanes. There is no obvious ongoing major merging activity, however there might be subtle signs of minor disturbances. The galaxy has a moderate blue color, possibly suggesting ongoing star formation, though this is less pronounced than in typical spiral galaxies. The galaxy's apparent magnitude indicates that it is intrinsically luminous despite its distance. The galaxy is fairly compact in size.
