The galaxy presents as a somewhat smooth, elliptical-like structure, with no apparent spiral arms or distinct disk features. Its color gradient suggests an older stellar population, trending towards the redder end of the spectrum. There is some indication of disturbance in the morphology, possibly suggestive of a minor interaction or ongoing merger event. A secondary, smaller object appears very close to the primary galaxy, potentially influencing its overall form. The central region of the galaxy displays a more concentrated brightness, indicating a higher density of stars or possibly an active galactic nucleus. The object appears quite round overall, with a slight elongation. Star formation appears to be relatively low. The galaxy is quite massive, with a low specific star formation rate.
