The galaxy presents as an elliptical morphology, though a disk component cannot be entirely ruled out due to the viewing angle. Its light profile appears relatively smooth, lacking prominent spiral arms or significant knotty structures indicative of intense star formation regions. A bright, concentrated central bulge dominates the overall structure, transitioning into a fainter, extended halo. Color gradients suggest a redder nucleus, potentially indicative of an older stellar population compared to the bluer, more diffuse outer regions, hinting at ongoing, though perhaps subdued, star formation within the galactic disk. There is some subtle indication of a minor disturbance. The overall appearance suggests this galaxy is somewhere between an elliptical and spiral galaxy. 
