The galaxy exhibits a smooth, elongated morphology, suggestive of an elliptical galaxy. The color profile appears to be relatively uniform, with a concentration of light towards the center, indicating a bulge-dominated system. There is a noticeable lack of distinct spiral arms or prominent dust lanes. The overall structure indicates a well-established system, potentially nearing the end of its star formation phase. Given the cigar shape, it is possible the galaxy is in the process of merging or has recently undergone a merger event, though there are no visible tidal tails or other major disturbances to indicate recent activity. The galaxy presents as a relatively undisturbed, evolved system.
