The galaxy presents a primarily smooth morphology, exhibiting a central bulge that appears relatively luminous and concentrated.  Its shape is largely in between round and elliptical. There is a slight hint of a disc structure, but it is not well-defined. The galaxy does not appear to be undergoing any major merging activity, although there are minor disturbances or asymmetries visible in the outer regions. These features suggest a possible interaction or accretion event in the galaxy's recent past, or perhaps just clumpy star formation. It exhibits a moderate level of star formation.
