The galaxy presents as a moderately luminous, elongated structure. Its central region exhibits a concentrated, bright, yellowish-orange hue, suggesting a potentially older stellar population and/or significant dust obscuration. The overall morphology appears relatively smooth, lacking prominent spiral arms or other distinct features. The outer regions of the galaxy appear fainter and somewhat diffuse, fading into the background sky. The galaxy's shape could be classified as elliptical, although a slightly distorted or irregular morphology cannot be ruled out based on this image alone. There is no immediately apparent evidence of active galactic nuclei activity or ongoing major star formation.
