The galaxy presents as an elongated, elliptical-type structure. The light distribution is generally smooth and centrally concentrated, with a gradual decrease in luminosity towards the outer edges. The central region exhibits a yellow-white hue, suggesting the presence of an older stellar population. There are no obvious spiral arms or dust lanes visible. The overall shape is cigar-like. There are no visible signs of recent or ongoing major mergers or significant disturbances in the galaxy's morphology. The galaxy is relatively compact.
