The galaxy presents as a moderately luminous object with a distinct elliptical morphology. The light distribution appears relatively smooth and centrally concentrated, suggesting a lack of significant spiral arm structures. The color profile exhibits a general trend from redder hues in the central regions to slightly bluer tints at the periphery, potentially indicating a radial variation in stellar population or dust content. No obvious signs of major mergers or tidal disturbances are apparent; however, subtle asymmetries or irregularities cannot be entirely ruled out. The overall appearance is consistent with a relatively evolved galaxy, potentially undergoing a period of quiescence in star formation activity.
