The galaxy appears as a centrally concentrated object with a smooth, somewhat circular morphology. It exhibits a distinct greenish-yellow hue, suggesting a moderate level of ongoing star formation. There is little evidence of significant spiral arm structure or pronounced disk features. The galaxy displays a slightly elongated shape, deviating marginally from a perfectly circular form. The central region shows a higher concentration of light, implying a substantial bulge component. No major mergers or tidal disturbances are readily apparent; however, there is a slight asymmetry in the outer regions suggesting potential minor gravitational interaction. The overall color and smooth features indicate a galaxy transitioning away from intense star formation activity, potentially evolving towards a more quiescent state.
