The galaxy presents a generally smooth and somewhat elliptical morphology. Its core exhibits a concentrated, bright yellow-white emission, indicative of an older stellar population. Moving outward from the core, the color transitions to a bluer hue, suggesting the presence of younger stars or ongoing star formation in the outer regions. The galaxy appears relatively undisturbed, with no obvious signs of recent major mergers or tidal interactions. Faint, diffuse features are present, hinting at a possible disk or extended halo.
