The galaxy presents as a centrally concentrated spheroid. It exhibits a relatively smooth, featureless morphology, indicating a lack of prominent spiral arms or strong bar structures. The light distribution appears dominated by an older stellar population, with a color gradient suggesting a higher concentration of older, redder stars toward the center. The overall roundness and lack of significant tidal features suggest a system that is not currently undergoing a major merger, though there might be a hint of a minor disturbance in the outer halo. The galaxy appears moderately luminous, consistent with a substantial stellar mass. Based on the observed color and smooth morphology, this galaxy is likely an elliptical or lenticular type.
