The galaxy presents as a centrally concentrated system with a smooth overall appearance. It exhibits an elliptical morphology, appearing elongated with a cigar-shaped profile. The light distribution suggests a gradual decline in brightness from the core outwards, characteristic of an elliptical galaxy.

There is no obvious presence of spiral arms or a distinct disk-like structure. A faint blue hue around the edge suggest the possibility of star formation, but not enough to define it as a spiral galaxy. The light is red-shifted, but the galaxy still displays light from the blue end of the spectrum. 

There is no indication of ongoing major mergers or significant tidal disturbances affecting the overall structure, however, this galaxy does look like a recent merging event may have taken place.
