The galaxy appears to be a relatively compact, elliptical system, exhibiting a smooth, centrally concentrated morphology. There is a marked absence of spiral arms or prominent disk features. The central region shows a bright, concentrated core, potentially indicating the presence of an active galactic nucleus (AGN) or a dense stellar population. The overall color appears redder, suggesting an older stellar population with lower levels of ongoing star formation. The galaxy shows a slight ellipticity, appearing somewhat flattened in shape. There is no indication of any major mergers or significant tidal disturbances.
