The galaxy appears as a relatively smooth, elliptical-like object with a concentrated central bulge. The light distribution is centrally peaked, with a gradual decrease in intensity moving outwards from the core. There is some subtle color variation, with the central region exhibiting a slightly yellower hue compared to the outer regions. The outer regions appear more diffuse and less structured with no obvious features. There is no evidence of a prominent disk, spiral arms, or significant dust lanes visible at this resolution. The overall morphology suggests a galaxy in the later stages of its evolution.
