The galaxy presents as a primarily smooth, elliptical structure. It exhibits a concentrated central bulge with a bright, yellowish core, indicating a population of older stars. The outer regions of the galaxy appear less defined, fading into the background with a slightly elongated shape, suggesting a cigar-shaped morphology. Faint hints of blueish light are observed in the outer edges, potentially indicating regions of recent, but low, star formation. There are no readily apparent spiral arms or significant dust lanes visible, and no signs of major mergers or interactions, though there may be minor disturbances visible in the morphology. Overall, the galaxy appears to be relatively quiescent.
