The galaxy presents a generally smooth appearance, lacking a highly defined spiral structure. The light distribution suggests a concentrated central bulge, surrounded by a more diffuse halo. The galaxy's color profile seems relatively uniform across its structure, with subtle variations. There is some indication of possible disturbances in the outer regions, although these features are not highly pronounced. The overall morphology points towards a galaxy undergoing, or having completed, a transition towards a more quiescent state, with limited ongoing star formation indicated by its color. The object appears significantly influenced by its internal processes and potentially by minor interactions with other galaxies.
