The galaxy presents as a complex system, exhibiting characteristics of both a spiral and an elliptical morphology. A dominant, relatively bright bulge-like structure is apparent, displaying a smooth, diffuse profile with a somewhat yellowish core. This suggests an older stellar population with a lower rate of star formation. Adjacent to this bulge, a significantly flattened disk is visible, oriented approximately edge-on to our line of sight. The disk exhibits a clear color gradient, appearing more reddish in hue than the central bulge. This indicates the presence of dust lanes and regions of ongoing star formation within the disk. There is evidence of morphological disturbance or tidal features, as the structure appears asymmetric.
