The galaxy presents a largely smooth morphology, with a high degree of central concentration. Its shape appears to be approximately elliptical, exhibiting a somewhat rounded form. There are no apparent signs of significant spiral arm structure or a prominent disk component. The overall color profile suggests a relatively red population, potentially indicating an older stellar population and a reduced rate of ongoing star formation activity. No signs of major mergers or tidal disturbances are observed, but there are subtle color changes between the center and outer regions, indicating a potential mass difference.
