The galaxy presents a smooth, elongated morphology, appearing cigar-shaped. Its light profile suggests a relatively uniform stellar distribution, lacking prominent spiral arms or a distinct central bulge. The galaxy exhibits a color gradient, transitioning from a bluish hue at the central region to a more reddish tint towards the outer edges. This color variation suggests a possible change in stellar populations, with younger, hotter stars concentrated in the core and older, cooler stars dominating the outskirts. There are no apparent signs of major mergers or significant tidal disturbances. The disk appears relatively undisturbed. Star formation appears to be suppressed in the galaxy.
