The galaxy appears as a single, mostly uniform body with a concentrated central region. The light profile suggests a smooth distribution, lacking any prominent spiral arms or distinct features associated with active star formation regions. It presents a largely elliptical morphology with a smooth light distribution, a nearly round shape, and a high degree of symmetry. Color gradients within the galaxy are subtle, with a slight central concentration of yellow light, indicating a potentially older stellar population. There is no apparent evidence of ongoing major mergers or significant tidal disturbances impacting the galaxy's structure. Faint wisps or extended diffuse light surrounding the central regions may exist, indicating past interaction or accretion events, but are not obvious at first glance. The overall color and morphology are consistent with a galaxy with relatively low current star formation activity.
