The galaxy presents as an elliptical or lenticular system, exhibiting a generally smooth morphology with little to no discernible spiral arm structure. The light distribution suggests a centrally concentrated spheroid component, with the brightest region indicating a prominent galactic nucleus. There appears to be a slight elongation in the galaxy's shape, trending toward a cigar-like morphology. Coloration is mostly uniform, displaying a yellowish or golden hue that is consistent with older stellar populations and relatively low current star formation. There appears to be a faint object to the right that may or may not be interacting with the primary galaxy.
