The galaxy presents as a relatively smooth, elliptical structure. The central bulge is prominent, exhibiting a bright, concentrated luminosity, suggesting a high density of older stellar populations. Moving outwards from the core, the light gradually diminishes, with a diffuse halo surrounding the central region. There is a subtle color gradient, with the core appearing slightly yellower or redder than the outer regions, possibly indicative of variations in stellar populations or dust content. No distinct spiral arms or prominent dust lanes are discernible, further supporting its classification as an elliptical galaxy. There is no evidence of significant tidal disturbances or interactions with other galaxies in its immediate vicinity. Overall, the galaxy appears to be a well-formed, quiescent system with a smooth morphology.
