The galaxy presents as a generally smooth, elliptical structure. The core displays a bright, concentrated luminosity, suggesting a high stellar density or the presence of an active galactic nucleus, though further spectral analysis would be needed to confirm the latter. The luminosity gradually decreases from the center outwards, forming a diffuse halo.

The galaxy exhibits a generally rounded morphology, with only slight deviations from a perfect circular shape. There is no clear evidence of a spiral arm structure or a prominent disk component. Faint tidal features may exist but is not a major contributor. The overall color index appears relatively uniform across the galaxy, hinting at a homogenous stellar population of primarily older stars. There is a slight asymmetry with a slight extension towards the upper portion of the image. Based on the color profile and morphology, this galaxy appears to be an early-type galaxy, likely an elliptical or lenticular system.
