The galaxy presents a somewhat elliptical morphology, displaying a smooth light distribution. It appears largely featureless, lacking prominent spiral arms or a distinct bar structure. The central region exhibits a higher surface brightness, indicating a concentration of stars towards the core, likely due to the presence of a supermassive black hole and bulge. The color gradient reveals a yellowish central region that transitions to bluer outer regions. The subtle color differences suggest varying stellar populations. The galaxy is isolated, with no obvious signs of tidal distortions or interactions with neighboring galaxies, though there appears to be minor light disturbances.
