The galaxy presents a generally smooth morphology, appearing as a flattened spheroid with a major axis of approximately 5 kpc. It exhibits a subtle central bulge, and a faint blue hue is noticeable. Irregular features suggest a recent or ongoing interaction, likely a minor disturbance or merger event. The light distribution indicates ongoing star formation within the galaxy, concentrated in the regions where a blue tint is noticeable. Based on the shape, the galaxy is likely an intermediate type, between elliptical and spiral.
