The galaxy presents as a relatively smooth, elliptical-like structure. There is a concentrated central bulge with a bright and diffuse glow. Moving outwards from the central bulge, the light gradually decreases in intensity, creating a gradient effect. There appears to be minimal substructure such as spiral arms or distinct dust lanes. The overall shape is generally rounded, lacking a prominent disk-like structure. There are no clear signs of ongoing mergers or major tidal disturbances affecting the galaxy's morphology. Overall, the galaxy appears to be a quiescent system, displaying characteristics of a mature galaxy with a large population of older stars.
