The galaxy exhibits a generally smooth morphology, appearing as a concentrated central bulge surrounded by a more diffuse halo. There is evidence of a disk-like structure, although it is not sharply defined and lacks prominent spiral arms. The color profile suggests a relatively evolved stellar population, with a yellowish hue dominating the central region, indicative of older, redder stars. The outer regions show a subtle bluer tint, possibly indicating some ongoing, albeit low-level, star formation. Overall, the galaxy appears relatively undisturbed, without major distortions or signs of ongoing mergers, though a minor disturbance might be present in its overall shape. The general roundness and lack of strong features suggest it may be an early-type spiral or a lenticular galaxy.
