This galaxy presents a predominantly elliptical morphology with a smooth, centrally concentrated luminosity profile. A notable feature is the presence of a subtle disk-like structure, evident by the faint flattening along the equatorial plane. The core of the galaxy displays a bright, concentrated region, possibly indicative of an active galactic nucleus or a dense stellar population. Faint, diffuse extensions are observed emanating from the main galactic body, suggesting the presence of stellar halos or tidal features.

The galaxy exhibits a color gradient, with the central region appearing bluer compared to the reddish outer regions. This may suggest a difference in stellar populations, with younger, hotter stars concentrated towards the core and older, redder stars dominating the outer regions. While the overall structure appears relatively undisturbed, there are subtle indications of minor morphological disturbances, potentially due to past or ongoing interactions. The galaxy does not show significant signs of major mergers or tidal disruptions.
