The galaxy presents as a centrally concentrated, elliptical-like object with a generally smooth appearance. The core region exhibits a yellowish-white hue, suggesting an older stellar population and possible dust obscuration. Moving outwards from the core, the galaxy fades into a bluish halo. This suggests the presence of a younger, bluer stellar population in the outer regions. The galaxy exhibits a slightly elongated shape, leaning towards a rounded form. There is a minor visual disturbance in the galaxy's morphology, which could be indicative of a recent or ongoing minor merger event. There is an absence of defined spiral arms or a clear disk structure.
