The galaxy presents a generally smooth and concentrated morphology. The central region appears to have a high concentration of older stars, exhibiting a yellowish hue, potentially indicative of an aging stellar population with relatively low ongoing star formation. The galaxy is approximately elliptical in shape, with a deviation from perfect circularity. A slight distortion or asymmetry may suggest minor tidal interactions or internal dynamic processes. Weak color gradients are observed within the galaxy, transitioning from a yellower core to slightly redder outer regions, though the image resolution limits detailed analysis.
