The galaxy presents as a generally smooth, elliptical-like object. It appears to be relatively round, with a high degree of central concentration of light. The core region exhibits a bright yellowish hue, indicative of a population of older stars, or potentially dust absorption. There is very little indication of spiral arms or disk-like structure. A slight deviation from perfect circularity is observed, hinting at a possible, though subdued, elongation or ellipsoidal shape. There's no readily apparent evidence of ongoing major mergers or strong tidal disturbances, and there's no indication of intense star forming regions. Overall, the galaxy seems consistent with a passively evolving system.
