The galaxy presents as an elongated, moderately luminous object with an estimated size of approximately 12 kiloparsecs. It exhibits a central bulge region that appears relatively smooth and contains primarily older stellar populations, indicated by its yellowish-orange hue. The galaxy also appears to have a weak disk component. A slight blue tint on one side of the disk component suggests some ongoing star formation, although this activity appears limited, as the overall color profile indicates a redder, more quiescent system. There appears to be some minor distortion from the smooth shape, which could be due to a minor gravitational interaction. Overall, the galaxy seems to be in a transitional phase, potentially evolving from a spiral-like morphology to a more elliptical, passive state.
