The galaxy presents as a relatively compact and luminous object. Its overall morphology appears smooth and elliptical, lacking well-defined spiral arms or a prominent disk structure. There is a noticeable concentration of light towards the center, suggesting a significant bulge component. 

The galaxy exhibits a color gradient, with the central regions appearing more yellow-reddish, indicating an older stellar population. Fainter blue light is possibly visible in its outer regions, suggesting the presence of younger stars, possibly indicative of some recent star formation.

There is a suggestion of possible tidal features or a minor disturbance in the galaxy's outer halo, which indicates possible interactions with another object or galaxy.
