The galaxy presents a somewhat amorphous, compact appearance. There is a bright central core, likely a nucleus. Proceeding outwards, faint diffuse emission surrounds this bright core, extending in a somewhat irregular fashion. The core exhibits a bluish-white hue, suggesting the presence of hot, young stars or active galactic nucleus activity. The surrounding halo of emission appears reddish, which could indicate older stellar populations, dust obscuration, or redshift effects. There appears to be some slight irregularity in the outer halo, which is potentially indicative of tidal interactions, or the aftermath of a minor merger. The galaxy is primarily smooth in appearance, without distinct spiral arm structures evident. 
