This galaxy presents as an elliptical morphology, exhibiting a smooth, centrally concentrated light distribution. The core region shows a high degree of luminosity, suggesting a dense stellar population. The overall color appears to be relatively redder, possibly indicative of an older stellar population with lower ongoing star formation. The galaxy displays a generally rounded shape with only slight deviations from perfect circularity. No prominent spiral arms or bar structures are discernible. There is no obvious evidence of major mergers or significant tidal disturbances in the immediate vicinity. The galaxy appears isolated.
