The galaxy presents a generally smooth morphology with a concentrated central bulge. The light distribution appears relatively uniform and lacks the distinct spiral arm structures or irregular features often associated with late-type galaxies. The color gradient transitions from a yellowish core to a redder periphery, suggesting a centrally concentrated population of older stars. There is a subtle hint of bluer light in the outer regions, which could be indicative of some recent, low-level star formation. Overall, the galaxy's structure points toward an elliptical or lenticular classification. There is no strong indication of ongoing merger activity or significant tidal disturbances. The axial ratio indicates it is neither perfectly spherical nor highly elongated, appearing closer to an elliptical galaxy of moderate ellipticity.
