The galaxy presents a generally smooth morphology, exhibiting a centrally concentrated structure. The core region is bright and appears yellowish-white, potentially indicating an older stellar population. Surrounding the core is a more diffuse, bluish halo. This suggests the presence of a younger, bluer stellar population in the outer regions, and may be indicative of ongoing star formation at a low rate.

The galaxy appears roughly round in shape, with a subtle elongation or asymmetry in the distribution of the bluish light. It is possible that this asymmetry is the result of a past minor interaction or disturbance, though the galaxy does not appear to be undergoing a major merger. 
