The galaxy presents a mostly smooth and rounded morphology. The core of the galaxy exhibits a strong concentration of light, appearing bright and yellowish in color. A more diffuse, extended halo surrounds the central region, fading in intensity. The halo exhibits a slightly bluer hue, suggesting the presence of a younger stellar population compared to the core. There are no prominent spiral arms or bar features visible. Evidence suggests a possible interaction or recent merger, with an irregular shape and an absence of central symmetry. It is experiencing relatively low star formation.