The galaxy presents as a largely featureless, smooth object. It exhibits a nearly round morphology, with minimal elongation discernable. There is a central concentration of light, suggesting the presence of a bulge. A faint, diffuse halo surrounds the central region. The overall color appears to be a slightly blue-white hue near the center, transitioning to a redder tint in the outer regions. This coloration may indicate ongoing star formation within the central bulge, with an older stellar population dominating the halo. There is no visually apparent spiral arm structure or significant dust lane absorption. The galaxy appears relatively undisturbed, with no obvious signs of recent major merger events. Subtle disturbances might be present, but there are no strong indications of tidal tails or other disruptive features.
