The galaxy presents as an elliptical morphology, with a smooth, centrally concentrated light distribution. There is minimal evidence of spiral arm structure or significant dust lanes. The core region appears to be relatively bright and yellow-ish, indicative of an older stellar population. The outer regions exhibit a subtle color gradient, appearing somewhat redder than the core, potentially suggesting a difference in stellar age or metallicity. The overall shape is somewhat elongated, but not extremely so. No significant tidal features or indications of ongoing major mergers are apparent, although there may be slight evidence of minor disturbance to the upper right of the galaxy.
