The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a yellowish hue, suggesting a population of older stars. There is a subtle extension of light on one side, perhaps indicating a faint tidal feature or a very weak spiral arm structure. The overall morphology appears elliptical or possibly lenticular, with a high degree of rotational symmetry. There is no strong evidence of active star formation, at least not at a rate sufficient to significantly alter the galaxy's color. It appears to be an evolved galaxy, potentially quiescent, and undergoing little to no major merging activity.
