The galaxy presents as an elongated, cigar-shaped structure, suggestive of an elliptical morphology. It exhibits a smooth, featureless appearance with no discernible spiral arms or distinct substructures. The central region displays a concentration of light, indicating a possible bulge or core. The color gradient transitions from a more yellow-orange core to a slightly fainter, redder hue in the outer regions. This color variation could imply a radial distribution in stellar populations, with older, redder stars dominating the outskirts, and a younger, hotter population within the center. There is no evidence of significant dust lanes or active star formation within the observed wavelengths, pointing towards a likely quiescent or passive galaxy. The overall texture indicates a high degree of homogeneity, with the lack of major disturbances suggesting a gravitationally relaxed system, and only minor disturbances.
