The galaxy presents as a relatively smooth and concentrated object. It appears elliptical in shape, with a high degree of roundness, as it lacks any discernible disk-like structure or significant elongation. The central region displays a pronounced concentration of light, suggesting a bright nucleus. The light profile decreases steadily with increasing radius, indicating a smooth distribution of stars. There is no evidence of spiral arms, bars, or significant dust lanes within this galaxy. The color appears to be moderately red, which could imply an older stellar population and low levels of on-going star formation. No signs of recent or ongoing mergers or tidal disturbances are visible.
