The galaxy appears to be a relatively smooth, centrally concentrated system. It exhibits a primarily elliptical morphology, with a high degree of roundness. The core region displays a yellowish hue, suggesting an older stellar population. The galaxy’s outer regions appear less defined, fading into the background sky. There is minimal evidence of spiral arms or a distinct disk structure. Very little to no signs of active star formation are present, aside from a small red region within the galaxy that may suggest minor star formation. No indications of major mergers or significant tidal disturbances are observed.
