The galaxy presents as an elliptical morphology, characterized by a smooth and centralized luminosity profile. The light distribution appears concentrated, with a bright, yellowish core gradually fading outwards. There is a discernible lack of distinct spiral arms or prominent dust lanes. The galaxy exhibits a subtle elongation, but otherwise lacks major disturbances in its overall structure, suggesting it is not currently undergoing a major merger event. Its reddish color suggests an older stellar population and comparatively low star formation rate.
