The galaxy presents as a smooth, elliptical structure with a notable central bulge. Its overall shape is elongated, resembling a cigar shape, with the major axis oriented approximately vertically in the image. The light distribution is concentrated towards the center, indicating a higher stellar density in the core. There is a gradual decrease in brightness as you move outwards from the nucleus. Faint disk or arm features are not visible. No signs of major mergers or significant tidal disturbances are apparent. The color appears generally redder, which suggests an older stellar population with relatively low current star formation activity.
