The galaxy appears to be an elliptical galaxy, characterized by a smooth, featureless morphology. It is elongated in shape, with the ratio of its major to minor axes suggesting a moderate ellipticity. The central region exhibits a higher surface brightness, indicating a concentration of stars toward the galactic nucleus. The color profile suggests a dominance of older stellar populations, evidenced by the redder hue compared to typical spiral galaxies. There is no discernible dust lane or spiral arm structure. There may be some minor disturbance to this galaxy as indicated by a companion galaxy.
