The galaxy presents as a lenticular or possibly elliptical structure, characterized by a smooth, relatively featureless light distribution. It exhibits a flattened, elongated morphology, suggesting a disk-like component viewed at a significant inclination. The central region displays a concentration of light, likely indicating a bulge component, while the outer regions fade gradually. The color gradient shifts subtly from a yellowish-white core to bluer tones towards the periphery. There is no apparent dust lane or spiral arm structure visible. Overall, the galaxy seems relatively quiescent in terms of ongoing star formation. There is no significant morphological disturbance detected, indicating it is most likely not undergoing a major merger, though there could be a minor interaction happening. 
