The galaxy presents as a roughly elliptical object, with a high degree of central concentration. There is a smooth distribution of light across the galactic body. The central region appears bright, suggesting a concentration of older stellar populations and potentially a supermassive black hole undergoing limited accretion. The light profile smoothly decreases with radial distance from the center. The morphology is mostly smooth with no apparent spiral arms or dust lanes visible in the image. The galaxy appears slightly elongated, but not significantly cigar-shaped. There is no indication of any major ongoing merger events or tidal disturbances, suggesting it is likely a relaxed system that may have had some minor interaction in the past. There is a hint of redder coloration towards the center and a bluer coloration toward the outskirts, suggesting ongoing star formation is limited.
