The galaxy appears as a moderately luminous, elliptical-shaped object with a relatively smooth texture. The light is primarily concentrated in the center, suggesting a high degree of central mass. The color gradient indicates the presence of a mix of stellar populations. The outer regions seem slightly elongated, but there is no clear evidence of a distinct disk structure or spiral arms. There are subtle irregularities that may suggest it could be undergoing a minor disturbance of some kind. However, the overall morphology suggests a relatively evolved galaxy with a substantial population of older stars.
