The galaxy presents an overall smooth morphology, with a generally elliptical shape but a slight deviation suggestive of a disk. The central bulge is bright and concentrated, appearing yellowish, which likely indicates an older stellar population. Fainter, bluer regions exist around the bulge, hinting at more recent star formation activity. There is some evidence of minor disturbances, such as tidal features, or it could be undergoing a possible minor merger or interaction with another galaxy, although further observations are needed to confirm this. The galaxy's overall color suggests it is at an intermediate redshift, meaning we are observing it as it was when the universe was younger.
