The galaxy presents as an elliptical morphology, exhibiting a relatively smooth light distribution without prominent spiral arms or a distinct bar structure. It appears to be moderately luminous, with a central bulge that dominates the overall brightness. The radial color gradient suggests the core is redder than its outer regions, which is indicative of an older stellar population concentrated in the galactic nucleus and a younger population with ongoing star formation in the outer regions. The shape is neither perfectly spherical nor highly elongated; it occupies an intermediate ellipsoidal form. There is only subtle evidence of any tidal disturbances or ongoing mergers, appearing largely undisturbed. Overall, the galaxy is a likely an evolved system exhibiting signs of a mature stellar population in the central region.
