This galaxy exhibits a generally smooth morphology, with an apparent lack of defined spiral arms or a prominent central bar structure. The light distribution suggests it is likely an elliptical galaxy or a lenticular galaxy viewed at a considerable angle. The object presents a moderate ellipticity, appearing somewhat cigar-shaped rather than perfectly round. A central bulge is evident, characterized by a yellowish hue that likely indicates an older stellar population. The outer regions exhibit a bluer tint, possibly due to a younger population of stars or ongoing, albeit mild, star formation activity. Subtle disturbances or minor irregularities may be present in the outskirts, suggesting a possible past interaction or minor merger event, however, the overall structure remains largely undisturbed. 
