This galaxy presents as a primarily smooth, elliptical-like structure. It appears elongated, exhibiting a cigar-like shape rather than a perfectly circular profile. A central bulge is clearly visible, characterized by a bright, concentrated core indicative of a high stellar density. The color gradient suggests a population of older stars dominating the bulge, transitioning to slightly bluer hues in the outer regions. No distinct spiral arms or significant dust lanes are discernible, reinforcing the classification of this galaxy as an elliptical. There is no obvious evidence of ongoing major mergers or significant tidal disturbances in its morphology.
