The galaxy presents as a largely featureless, elliptical-like object. The core region exhibits a high degree of luminosity, suggesting a concentrated distribution of stellar mass. The luminosity decreases gradually from the core outwards. There is some indication of faint, extended structure surrounding the central region, though it appears smooth and lacks the distinct spiral arms or irregular morphologies often associated with actively star-forming galaxies. The color profile suggests that the galaxy is composed of relatively old stellar populations, as evidenced by the predominantly redder hue of the outer regions compared to the core.
