The galaxy presents as a single, relatively smooth object. Its overall shape is round to slightly elliptical. There is a noticeable central bulge that is bright and concentrated, displaying a yellowish hue. The outer regions appear less luminous with a gradual fade towards the edges, indicative of a decreasing stellar density. No distinct spiral arms or significant dust lanes are discernible. There is a subtle asymmetry to the galaxy's light distribution, potentially suggesting minor gravitational interactions or past merger events, though no major disturbances are immediately apparent. The color profile suggests a population dominated by older stars, contributing to the overall yellow-red color of the galaxy. Star formation activity appears to be low.
