The galaxy presents an elliptical morphology, appearing largely smooth and spheroidal in shape. The central bulge is a prominent feature, exhibiting a high concentration of luminosity. The light emanating from this region suggests an older stellar population. There is the suggestion of a disk and some evidence of faint spiral arm structure, albeit poorly defined. A region of blue light is observed at the edge of the galaxy that may represent ongoing star formation. Overall, the galaxy appears to be a relatively massive system, potentially undergoing some minor interaction or disturbance given the slight asymmetry of the outer regions. There is no pronounced evidence of a major merger event or tidal disruption, but it shows signs of a dynamic environment.
