The galaxy appears as a centrally concentrated, elliptical-like structure with a smooth overall morphology. There is a dominant bulge component that is bright and yellowish in color, indicating a population of older stars. The light distribution fades gradually from the center outwards, with no discernible spiral arm structures or prominent dust lanes. There is a slight elongation, making it appear somewhat "in between" round and cigar-shaped. There is no evidence of any major mergers or significant tidal disturbances in the immediate vicinity. The overall appearance suggests a relatively quiescent system with little ongoing star formation. The blue color seems subdued or absent, implying a lack of young, massive stars.
