The galaxy presents as a relatively smooth, elliptical-like structure. The light distribution suggests a centrally concentrated bulge, with a gradual decrease in luminosity towards the outer regions.  The core appears bright and concentrated, with a hint of bluer light. There's a subtle, extended halo or envelope surrounding the main body, indicating older stellar populations. Overall, the galaxy exhibits a fairly regular morphology, with no clear signs of recent major mergers or tidal disturbances, however there is possible slight distortion in one area. There's a possibility of some dust content due to slightly redder color in some regions, though not very prominent. The galaxy appears to be at an observable distance where features can be recognized.
