The galaxy exhibits a generally smooth morphology. It displays an elongated, cigar-like shape. The central region is the brightest and appears more concentrated, with a gradual decrease in luminosity towards the outer edges. A subtle color gradient is present, with the core showing a slightly redder hue, transitioning to a bluer tint in the more diffuse outer regions. There is no strong evidence of distinct spiral arm structures, major disturbances, or ongoing mergers within the visible portion of the galaxy. Overall, the galaxy presents as an elliptical or lenticular type, displaying a fairly well-defined, smooth profile.
