The galaxy presents a largely smooth morphology, appearing elliptical in shape. Its overall color profile is consistent with an older stellar population, exhibiting a yellow-orange hue concentrated towards the galactic center, with a lower concentration of blue stars. Faint, diffuse extensions or tidal features are potentially present, but not well-defined, suggesting either past minor merger activity or internal dynamical processes. There is little to no evidence of prominent spiral arms or significant ongoing star formation. The galaxy is moderately luminous, with a bright central bulge, suggesting the presence of a supermassive black hole actively feeding at its center. The overall appearance indicates a galaxy undergoing, or having already undergone, a transition from a star-forming spiral to a quiescent elliptical galaxy.
