The galaxy presents a largely smooth, elliptical morphology, appearing nearly round in projection. A concentrated, bright central bulge dominates the structure, surrounded by a fainter, more diffuse halo. There is minimal evidence of spiral arms or a distinct disk component. The overall color index suggests the presence of an older stellar population, with little ongoing star formation visible. Subtle irregularities in the outer regions may indicate a past minor interaction or disturbance, but the overall structure is relatively undisturbed.
