The galaxy presents a largely smooth morphology, appearing elliptical in shape with a notable elongation. Its color gradient transitions from a brighter, more concentrated central region towards fainter edges. The central region is significantly brighter, suggesting a higher stellar density, likely representing the bulge. There is little to no visible structure such as spiral arms or dust lanes. The galaxy has a relatively homogenous color profile, with subtle color variations across its extent. Overall, the galaxy appears to be an evolved system with a relatively quiescent star formation rate.
