The galaxy presents as a centrally concentrated, luminous object. It exhibits a predominantly smooth morphology, with minimal evidence of spiral arm structure. The central region of the galaxy appears bright, indicative of a possible active galactic nucleus or a high concentration of stars. A faint, extended halo surrounds the central region, suggesting the presence of an older stellar population. There are slight color variations visible, with a bluer hue concentrated in the center and more red coloration in the halo. The ellipticity of the galaxy suggests it is somewhere between a circular and a cigar shape when viewed from our angle. There is no immediately apparent evidence of a major merger event, though minor disturbances are not ruled out. The color and morphology collectively suggest that this is most likely a galaxy somewhere in the transition between a spiral and elliptical galaxy. Overall, the galaxy appears to be a relatively massive system with suppressed star formation.
