The galaxy appears to be relatively compact, exhibiting a bright, centrally concentrated core. The morphology suggests a primarily smooth structure, with a distinct lack of prominent spiral arms or a well-defined disk. A faint, diffuse halo surrounds the bright core, extending outwards in a somewhat irregular shape. There are possible signs of minor tidal disturbances or asymmetries in the outer regions of the halo, potentially indicative of a past or ongoing interaction with another galaxy, or perhaps an internal disturbance. Color variations suggest possible active star formation. A blue tint around the core suggests the presence of younger, hotter stars.
