The galaxy presents as a centrally concentrated, elliptical-like structure. The core exhibits a high degree of luminosity, suggesting a dense concentration of stars or an active galactic nucleus. The light from the central bulge appears yellow-red, possibly indicating an older stellar population. The galaxy fades out with distance from the core in a relatively smooth profile. There is no apparent disc structure, spiral arms, or significant dust lanes. The galaxy appears generally isolated with no signs of major tidal disturbances or mergers visible.
