The galaxy presents a generally smooth, elliptical morphology with an overall rounded appearance. There is little evidence of prominent spiral arm structures or significant dust lanes. The color profile suggests a redder core, potentially indicative of an older stellar population concentrated towards the center. The galaxy appears fairly isolated, with no immediately apparent major tidal features or nearby merging companions, although a slight distortion in the outer isophotes may suggest a minor interaction. The galaxy's light distribution fades gradually from the core, indicating a relatively homogenous stellar distribution within the observed radius. The overall impression is of a well-formed, relatively undisturbed elliptical galaxy.
