The galaxy presents as a relatively smooth, centrally concentrated object with a slightly elliptical morphology. A dominant, bright, yellowish core region gradually fades into a more diffuse outer halo. There is little evidence of distinct spiral arm structures or significant dust lanes. The color gradient suggests a possible aging stellar population in the core with bluer regions in the outer portions, potentially indicative of ongoing, though perhaps relatively low, levels of star formation. The overall appearance is largely undisturbed, with no obvious signs of major merger activity or tidal features. Subtle asymmetry is observed but does not detract from the overall smoothness.
