The galaxy presents a primarily smooth morphology, suggestive of an elliptical or lenticular type. Its central region exhibits a concentrated, bright, yellowish hue, indicating a likely older stellar population. The galaxy's light profile seems to fade gradually towards the outer regions, where a hint of a disk-like structure is faintly discernible. The outer regions present a bluer color, potentially indicating regions of more recent star formation. There are no obvious signs of major mergers or strong tidal disturbances, although subtle asymmetries could imply minor past interactions. The overall shape is generally rounded, with only a slight deviation towards a more elongated form. Based on these observed features, this galaxy appears to be a massive system, likely past its peak of star formation, with a significant population of evolved stars, but potentially still harboring localized star formation in the outer disk regions.
