The galaxy presents a morphology that leans toward a smooth, elliptical form, yet exhibits subtle features indicative of a disk-like component. It appears mostly rounded in shape, with a slight elongation. The central region of the galaxy displays a concentrated, bright core, possibly indicative of an active galactic nucleus or a dense stellar population. Moving outward from the core, the light becomes more diffuse. There is a hint of blue-ish light around the edges of the galaxy, that may signify ongoing star formation. Overall, it appears to be a somewhat massive galaxy, undergoing a degree of star formation. There is no obvious evidence of a recent major merger event, though minor tidal disturbances cannot be entirely ruled out.
