The galaxy presents as a largely spheroidal object with a high degree of central concentration. Its color profile indicates a higher luminosity in the redder bands, transitioning to a bright yellow-white core. This suggests a relatively older stellar population dominating the galaxy's composition, which implies ongoing, but diminished star forming activity. The smooth, round morphology is indicative of an elliptical galaxy, or possibly a lenticular galaxy observed face-on. There is no apparent spiral arm structure, and the light is smooth without strong irregular features or significant disturbances due to merging or interactions.
