The galaxy presents a moderately bright, centrally concentrated morphology. The core region exhibits a yellowish hue, suggesting the presence of older stellar populations. Moving outwards from the center, the color gradually shifts to a bluer tone. This color gradient may indicate ongoing star formation in the outer regions of the galaxy, or younger stellar populations residing there.

The overall shape is generally smooth and elliptical, appearing somewhere between perfectly round and slightly elongated. There is little evidence of distinct spiral arm structure or a prominent disk component. There are no obvious signs of major interactions or mergers. There may be some minor disturbances in the galaxy's outer regions. The galaxy is plausibly a disk galaxy that is being viewed at a relatively high inclination angle. 
