The galaxy exhibits a generally smooth morphology, suggestive of an elliptical or lenticular type. The light distribution appears relatively uniform across the galaxy's body. The core is distinctly brighter and more concentrated, appearing nearly spherical. Moving outwards, the light gradually diminishes into the surrounding halo. There is a subtle color gradient, with the core displaying a more yellowish/reddish hue, possibly indicating an older stellar population and/or significant dust obscuration. Fainter bluish tinges may be present in the outer regions, indicating younger stars may be present. There is no clear evidence of spiral arms or other disk features, and no significant morphological disturbances are apparent.
