The galaxy presents an overall smooth appearance, suggesting an elliptical morphology. It exhibits a slightly elongated shape, appearing cigar-shaped. No distinct spiral arms or disk-like structures are visible, further supporting an elliptical classification. The color profile indicates a relatively blue hue, suggesting the presence of a younger stellar population, though the overall smoothness implies that star formation is likely suppressed within the galaxy. There is no indication of tidal disturbances or ongoing mergers from its morphology, but there is the slight chance of minor disturbance within the system. The overall morphology is consistent with an elliptical galaxy undergoing a period of quiescence, but still exhibiting some ongoing, though likely low, star formation activity.
