The galaxy presents as a centrally concentrated, elliptical-like object. It exhibits a smooth, diffuse light profile with a gradual decrease in luminosity from the center outwards. The core region appears a yellow-orange hue, likely indicating an older stellar population. Faint blue fringes can be detected around the central area, indicating possible star formation areas. There is a minimal presence of distinct spiral arm structures or prominent dust lanes. Based on the subtle distortions detected, it is possibly in a stage of minor interaction or disturbance. Its overall morphology indicates a lack of major ongoing merging events.
