The galaxy presents as an elliptical morphology, exhibiting a smooth, featureless structure with a pronounced central bulge. The object appears elongated, displaying an axis ratio that suggests a classification tending toward the 'in between' shape category, rather than perfectly round or strongly cigar-shaped. Color gradients suggest a more intense concentration of older stellar populations in the center, graduating to bluer, potentially younger stars in the outer regions, although the limited resolution makes it difficult to ascertain distinct spiral arm features. There is no immediately obvious indication of recent major merger activity or strong tidal disturbances, with the overall structure appearing relatively relaxed. The galaxy displays a redder hue overall which may indicate either an aging stellar population or significant dust extinction.
