The galaxy presents as a flattened, ellipsoidal structure, likely a disk galaxy viewed at a significant inclination. The central region exhibits a concentrated luminosity, suggesting the presence of a prominent galactic bulge. The color profile indicates a redder core region that fades into bluer tones in the more diffuse outer regions. There are no prominent spiral arms or distinct dust lanes visible in this image. The overall structure appears relatively undisturbed, showing no strong indications of recent major merger events or tidal interactions. The galaxy appears moderately massive, with low star formation compared to its estimated mass. It is mostly smooth, with a slight cigar shape.
