This galaxy presents as a relatively smooth, centrally concentrated object. It exhibits an elliptical morphology, appearing largely featureless without prominent spiral arms or a distinct bar structure. The light distribution suggests a high degree of radial symmetry. The central region shows a bright, yellowish core, likely indicative of an older stellar population. Surrounding this core, a bluish halo extends outwards, suggesting the presence of some younger, bluer stars, although their contribution to the overall light is subdued. There are no obvious signs of recent major mergers or significant tidal disturbances in its structure. A subtle asymmetry in the outer regions may indicate a minor interaction or an internal process affecting its shape.
