The galaxy presents as an elliptical or lenticular type, exhibiting a generally smooth and concentrated light profile. The core region is characterized by a bright, yellowish hue, suggesting a population of older stars. A subtle color gradient is observed moving outward from the center, shifting from yellow towards a slightly redder tinge in the outer regions, potentially indicating an aging stellar population and diminished ongoing star formation. The galaxy appears somewhat elongated with a faint disk-like structure. There is no evidence of significant tidal disturbances or active mergers. The overall morphology suggests a relatively evolved system.
