The galaxy presents as a somewhat elliptical structure with a smooth, concentrated central bulge. It appears largely featureless in the available imagery, with no discernible spiral arms or prominent dust lanes. The light distribution suggests a relatively old stellar population, with a redder hue dominating the color profile, particularly in the central regions. The galaxy exhibits a moderately high degree of ellipticity and is oriented with its major axis at roughly a 90-degree angle. The outskirts of the galaxy appear faint and diffuse, gradually fading into the background sky. There is no indication of any significant ongoing star formation, suggesting a passively evolving system. Overall, the galaxy appears to be a well-established elliptical galaxy at an intermediate redshift.