The galaxy presents as a relatively compact and luminous object. The morphology appears to be largely spheroidal, with a smooth, centrally concentrated light distribution and minimal discernible disk features. The galaxy exhibits a yellowish-white hue in its core region, potentially indicative of an older stellar population dominating the central region. Fainter blue light is noticeable around the core, suggesting the presence of younger stars and/or ongoing star formation in the outer regions of the galaxy, though at a subdued rate. No strong evidence of spiral arms or bar structures is apparent. The galaxy appears largely undisturbed, with no signs of major mergers or significant tidal features. There are some very minor disturbances nearby the edges of the galaxy, indicating some possible smaller mergers in its past. The overall impression is that of a mature galaxy, likely an elliptical or early-type spiral with a relatively quiescent star formation history.
