The galaxy presents as a moderately luminous, centrally concentrated object. Its overall structure appears smooth, with a gradual decline in surface brightness from the core to the outer regions. The core exhibits a yellowish to reddish hue, possibly indicative of an older stellar population or dust obscuration. Fainter bluish-greenish light surrounds the core and is likely from a population of younger, hotter stars, or ionized gas. There is no obvious spiral arm structure or distinct disk features visible in this image. The galaxy's ellipticity is low, suggesting a near-spherical or slightly oblate shape.
