The galaxy presents as a relatively smooth, disk-like structure seen at a slight angle. Its central region displays a concentrated brightness, indicative of a significant stellar population or possibly an active galactic nucleus. The inner bulge exhibits a yellowish-orange hue, suggesting an older stellar population with a lower rate of star formation. Fainter, bluer regions are present in the outer disk, potentially indicating areas of more recent star formation, though the structure is ill-defined. Overall, the galaxy's morphology suggests it is transitioning from a spiral towards a more lenticular or elliptical form. There is some evidence of minor disturbance on the outer edges of the disk, potentially from a past merger event.
