The galaxy presents as having a prominent bulge with a smooth, elliptical morphology. The central region exhibits a yellowish hue, suggesting an older stellar population. A fainter, bluer disk component is observed, extending outwards from the bulge. The disk appears somewhat disturbed or possibly interacting with a companion. The overall structure suggests it is transitioning from a spiral galaxy to an elliptical, possibly due to a past merger event that has disrupted the disk's structure and reduced ongoing star formation. The galaxy exhibits a low rate of star formation. The galaxy is a significant distance away from our own. The bulge seems to dominate the overall luminosity.
