The galaxy presents an overall elliptical morphology. The central bulge exhibits a concentrated brightness with a yellowish hue, suggestive of an older stellar population. Surrounding the core is a disk-like structure, less luminous, with a blue-green color. The outer region fades gradually into the background sky. The overall smooth appearance indicates it may be an early-type spiral, possibly an Sa, although no distinct spiral arm structures are clearly visible within this imaging. There might be a small disturbance or asymmetry within the outer disk, but additional deep imaging would be required to determine if the galaxy is currently undergoing a minor merger event. The galaxy is neither perfectly round nor highly elongated.
