The galaxy presents as a slightly elongated, disc-like structure. Its overall color profile suggests an older stellar population, with a dominant yellowish-orange hue in the central region. The outskirts of the galaxy display a faint bluish tint, potentially indicating pockets of more recent, albeit subdued, star formation activity. There are no clearly defined spiral arms; the light distribution appears relatively smooth and diffuse across the disk. The galaxy may be undergoing some minor gravitational interaction or disturbance based on subtle irregularities observed in its overall shape, but it appears mostly stable. The core of the galaxy exhibits a concentration of light, suggesting the possible presence of a galactic bulge.