The galaxy presents as a relatively compact object, displaying a roughly elliptical morphology. It appears largely smooth in structure, with a significant concentration of light towards the center, suggesting a prominent bulge.

There is a subtle color gradient across the galaxy, with the central region exhibiting a slightly bluer hue compared to the outer regions, which appear redder. This could indicate ongoing or recent star formation activity concentrated within the central region, or a difference in stellar population.

A faint, diffuse halo may be present, extending outwards from the main body of the galaxy.

There appears to be some minor disturbance of the galaxy's morphology, potentially caused by a recent merger.
