The galaxy presents with a generally elliptical morphology, displaying a smooth structure overall with some subtle internal features. A bright central region suggests a concentration of older stars or possibly an active galactic nucleus, though further spectroscopic data would be required to confirm the latter. Fainter, bluer regions extending outward from the core indicate the presence of more recent star formation within the disk. The galaxy does not appear perfectly isolated, displaying some asymmetry and possible tidal features hinting at a past or ongoing interaction with a companion galaxy.
