The galaxy presents a largely smooth and rounded morphology. The light profile appears centrally concentrated, exhibiting a gradual decrease in luminosity from the core outwards. There is no obvious spiral arm structure or bar visible. Color gradients suggest the core region is populated by an older stellar population. The outer regions exhibit a bluer hue, potentially indicating recent or ongoing star formation activity, though the resolution is insufficient to discern distinct star-forming regions. There is no indication of any major mergers or tidal disturbances. Minor disturbances are possible, though uncertain. The overall appearance suggests a galaxy that is tending towards a more evolved and quiescent state.
