The galaxy presents as a moderately inclined disc, elongated in shape. It displays a centrally concentrated brightness profile, indicating a bulge component. The outer regions of the disc show a smoother texture, with hints of spiral arm structure. There is a subtle color gradient, transitioning from a bluer central region, suggesting recent or ongoing star formation, to slightly redder outer regions, potentially indicative of an older stellar population. Overall, the galaxy appears relatively undisturbed with no obvious signs of major merging activity.
