The galaxy presents as a faint, elongated object with a moderately smooth appearance. There is a subtle, disk-like feature visible, though it is not sharply defined. A slight asymmetry in the light distribution is suggestive of a possible minor gravitational disturbance or interaction. No prominent spiral arms are discernible, nor is there evidence of a recent major merger event. The color profile suggests a mix of stellar populations, with a possibly dominant older population contributing to its overall yellow-red hue. The estimated physical size is approximately 11 kpc in radius. The light distribution shows the majority of light concentrated in its center. The overall morphology points towards a classification somewhere between a smooth elliptical and a disk-dominated spiral galaxy, hinting at a galaxy that may be in transition or has undergone past interaction events.
