The galaxy presents a generally smooth, elliptical morphology. The central region exhibits a high concentration of light, appearing yellowish-white, suggestive of an older stellar population. A faint, diffuse disk is visible, with a bluish hue, extending beyond the central bulge. This disk may contain regions of active star formation. The galaxy appears to be undergoing some tidal disturbances, with a slight asymmetry visible in the outer regions of the disk. There may be a minor interaction or a past merger event influencing its morphology. Overall, the galaxy appears to be in a transitional phase, potentially evolving from a spiral-like structure toward a more elliptical morphology.
