The galaxy presents a generally smooth morphology, with a concentrated central bulge exhibiting a bright, whitish-yellow hue. A faint, diffuse disk surrounds the bulge, displaying a bluish tint, which may be indicative of ongoing star formation within the galactic plane. The galaxy appears mostly circular in shape, though subtle distortions hint at possible gravitational interactions with other galaxies. There may be signs of minor disturbances in the overall structure. No prominent spiral arms or bars are discernible. The galaxy appears relatively isolated, suggesting it is not currently undergoing a major merger event.
