The galaxy presents a primarily smooth morphology, exhibiting a concentrated central bulge with a more diffuse surrounding halo. The color gradient suggests an older stellar population dominating the core, evidenced by the yellowish hue. Fainter, bluer regions appear sporadically in the outer regions of the halo. There is a subtle indication of a flattened disk-like structure, though without distinct spiral arms. No obvious signs of major mergers or significant tidal disturbances are apparent, though there are very faint, asymmetric features emanating from the galaxy that could be the remnants of a minor disturbance. The galaxy is likely a fairly massive system, given its overall brightness. Its quiescent star formation rate is consistent with a late-type galaxy transitioning into an early-type galaxy.
