The galaxy presents as a somewhat irregular, centrally concentrated object with a moderate angular size. The core region exhibits a bright, compact morphology, suggestive of a dense stellar population or potentially an active galactic nucleus. A faint, diffuse halo of lower surface brightness extends outwards from the central region, but is asymmetrical. A slight disturbance is visible in the halo's morphology, perhaps indicating a minor interaction or past merger event. The overall color of the galaxy appears to be dominated by bluer wavelengths, though some redder regions are also present along the periphery.
