The galaxy presents a generally smooth morphology, appearing as an elongated, elliptical-like structure. A concentrated central bulge exhibits a yellowish hue, suggesting an older stellar population. Moving outward from the core, the galaxy fades in intensity with a bluish tint. This is indicative of a fainter, more dispersed distribution of stars with ongoing star formation. There are no clear signs of prominent spiral arms or distinct features. The overall structure suggests a relatively evolved system that is not undergoing an active merger, with only minor disturbances, if any, to its smooth light distribution.
