The galaxy presents a roughly elliptical morphology, appearing somewhat compact. Its central region exhibits a high degree of luminosity, characterized by a cyan coloration, suggesting substantial ongoing star formation or an active galactic nucleus. The color becomes redder further away from the center. There is some degree of disturbance or irregularity in its shape. The galaxy appears to be mostly smooth, with no spiral arms or disk features distinctly visible. There is only a minimal indication of a potential ongoing merger. The halo surrounding the galaxy displays a radial color gradient.
