The galaxy presents a somewhat smooth, yet complex structure. It appears predominantly elliptical, with a concentrated central bulge that exhibits a yellowish hue, suggestive of an older stellar population. Faint spiral arm structures appear to emanate from the core, though they are not sharply defined. They give the overall impression of a galaxy that has likely undergone some disturbances, such as past interactions or minor mergers with another galaxy. The lack of strong blue color in the arms suggests a relatively low rate of recent star formation. The galaxy displays an intermediate inclination, allowing a partial view of its morphological features. Overall, this galaxy appears to be undergoing transition from a spiral to a more elliptical type.
