The galaxy presents as a relatively smooth, elliptical-like structure. Its overall shape is elongated, appearing somewhat flattened or "in between" round. A bright, concentrated central bulge is apparent, suggesting a high density of stars in the core. The light distribution decreases steadily from the center outwards. The galaxy exhibits a faint blue hue across its structure, particularly in the central area. A large portion of the galaxy is a more reddish color. There are no prominent spiral arms or bar structures visible. There are no signs of major disturbances or mergers. Overall, the galaxy appears to be a relatively isolated, well-defined, elliptical galaxy with signs of star formation.
