The galaxy presents as a largely smooth and rounded structure, exhibiting a concentrated central bulge with a diffuse halo. Its color profile indicates an older stellar population, appearing more yellow/orange than blue. There is little evidence of spiral arms or significant dust lanes, implying a more evolved system. There are no apparent signs of active galactic nuclei or tidal disturbances indicating major interactions. Overall, the galaxy appears to be an elliptical or lenticular galaxy, characterized by a lack of ongoing star formation and a well-mixed stellar population.