The galaxy presents as a flattened spheroid, exhibiting a yellowish-white hue indicative of a likely older stellar population. There is a subtle indication of a disk-like structure, with a slight elongation observed along one axis. The galaxy's light distribution appears relatively smooth and centralized, without prominent spiral arms or significant patchy star-forming regions immediately discernible. There is little sign of a central bulge, or a clearly defined nucleus. The overall structure suggests a possible transition between a spiral and elliptical galaxy. It is likely a massive galaxy with a moderate star formation rate. The shape is primarily rounded, and the galaxy does not appear to be undergoing any major merging activity, nor does it show signs of significant tidal disturbance.