The galaxy presents an elliptical morphology, with a smooth, diffuse light distribution. The core exhibits a yellowish hue, suggestive of an older stellar population. The outer regions fade into a bluer tint, potentially indicating the presence of younger stars or ongoing star formation, albeit at a low rate. No distinct spiral arms or bar structures are discernible. There is no significant evidence of major mergers or tidal disturbances, though a faint, asymmetrical glow on the outer edges of the disk may indicate minor disturbances. The galaxy's overall structure appears relatively undisturbed and quiescent.
