The galaxy presents as a relatively compact, elliptical-like system. Its light profile appears smooth and centrally concentrated, with a gradual decrease in luminosity outwards from the core. The core is of a yellow-ish hue, suggesting an older stellar population dominating the central regions. There's little evidence of spiral arms or significant dust lanes. The isophotes appear mostly round. There is no apparent signs of active galactic nuclei activity in the center or evidence of recent major mergers or tidal disturbances based on the morphology.
