The galaxy presents a disk-like morphology, viewed at a significant inclination. A central bulge is apparent, exhibiting a yellowish hue, suggestive of an older stellar population. The disk is characterized by a bluer color gradient, indicating the presence of younger, hotter stars and potential ongoing star formation. The disk structure appears somewhat disturbed or irregular, with hints of faint tidal features or asymmetries, possibly indicative of a past or ongoing interaction with another galaxy. The light distribution is not uniform, showing some clumpy regions within the disk, which could correspond to star-forming regions. Overall, the galaxy appears to be in an intermediate stage of evolution, exhibiting characteristics of both a spiral and an elliptical galaxy.
