The galaxy presents an overall elliptical morphology. The light distribution appears relatively smooth, indicating a lack of significant spiral arms or prominent dust lanes. The central region exhibits a brighter concentration, possibly indicative of an older stellar population or the presence of an active galactic nucleus, though the resolution makes this difficult to definitively determine. There is a hint of structural asymmetry in the core region, with two bright knots that are close to each other. The colour index suggests a relatively evolved stellar population, with a yellow-red hue dominating the galaxy's appearance. This is consistent with a galaxy where star formation has either ceased or is occurring at a low rate. Some distortions exist, indicating this galaxy may be experiencing minor disturbances or potentially have been through a merger. The mass estimate indicates that it is a massive galaxy, with a strong gravitational field.
