The galaxy appears as a singular, luminous object with a generally smooth morphology. Its color profile indicates a strong red component in the visible spectrum. No spiral arms or distinct disk features are readily discernible; the light is concentrated towards the center and fades gradually outwards, suggesting an elliptical or lenticular morphology. The overall structure implies a system that is relatively quiescent with a low star formation rate, likely dominated by an older stellar population. There's no visual evidence of any major mergers or tidal disturbances affecting the system's shape, and the galaxy appears mostly isolated and undisturbed.
