The galaxy presents a predominantly smooth morphology, with a high degree of central concentration. Its overall shape appears nearly circular, with a slight tendency toward an elliptical form. The galaxy exhibits a prominent bulge component that dominates its central region, exhibiting a yellowish-white hue, suggesting an older stellar population. The outer regions display a gradual decrease in luminosity, with faint extensions that are difficult to discern from the background noise. No spiral arm structures or distinct dust lanes are visible. The lack of obvious disturbances suggests that the galaxy is not currently undergoing any major merging events or strong tidal interactions. Overall, the galaxy appears to be a relatively undisturbed, evolved system. The galaxy's color is largely homogenous, lacking significant variations that would indicate prominent regions of on-going star formation.
