The galaxy exhibits a pronounced ellipsoidal morphology, appearing as a flattened spheroid when viewed in this orientation. It displays a smooth overall light distribution, with a gradual increase in brightness toward the central region. The core is somewhat indistinct and blends gradually into the surrounding bulge.

There is a distinct color gradient from the central bulge to the outer regions. The core appears to exhibit a yellowish to reddish hue, suggesting an older stellar population likely dominated by evolved stars. The outer regions have a somewhat bluer tinge in comparison, which may indicate the presence of more recent star formation activity.

No prominent spiral arm structures or other notable features are easily discernible. The lack of well-defined substructures may indicate that this galaxy is an early-type galaxy in the process of transformation. There are hints of minor disturbances in the outer edges, but it does not appear to be currently undergoing a major merger.
