The galaxy presents a generally smooth and rounded morphology. The central region exhibits a concentrated, bright core, possibly indicative of an active galactic nucleus or a dense stellar population. Moving outward from the core, the galaxy displays a gradual decline in surface brightness. The color profile suggests an older stellar population, with a reddish-yellow hue dominating. There is little evidence of spiral arms or significant dust lanes within the observed structure. A slight asymmetry, along the horizontal axis, may hint at minor tidal interactions, but the overall structure appears relatively undisturbed.
