The galaxy presents as a relatively smooth, elliptical-like structure with a bright, concentrated central bulge. Its overall shape appears to be somewhere between round and elongated, exhibiting a slight cigar-like morphology. There are no discernible spiral arms or prominent disk features visible. The light distribution indicates a high degree of central concentration, with a gradual decrease in luminosity outward from the core. No major disturbances or merging events are obviously apparent within the galaxy's structure; the galaxy may be experiencing minor disturbance. The galaxy appears to exhibit ongoing star formation.
