The galaxy presents an elliptical morphology, appearing as a smooth, centralized concentration of light. It exhibits a yellow-red hue which suggests an older stellar population. The light distribution decreases gradually from the core outwards, indicating a high Sersic index, which is consistent with an elliptical galaxy classification. The overall shape is elongated, with a major to minor axis ratio of approximately 0.7. There is no indication of spiral arm structures or significant dust lanes. No notable tidal features or major disturbances are observed suggesting it has not undergone a major merging event recently.
