The galaxy presents as a slightly elliptical, centrally concentrated object. It has a smooth overall appearance, lacking any distinct spiral arm structures or prominent dust lanes. The central region exhibits a yellowish-white hue, which may indicate an older stellar population. This core gradually transitions into a bluish halo which could indicate areas of recent star formation. The galaxy exhibits a faint, diffuse, and moderately compact structure with no signs of a major ongoing merger. Slight asymmetry in its shape suggests a possible minor disturbance event, but the object appears largely relaxed and undisturbed.
