The galaxy presents as a moderately luminous, elongated structure. Its overall color profile appears yellowish-white, suggesting a population dominated by older stars, though the presence of some blueish color indicates the presence of younger stars in certain areas. The galaxy exhibits a smooth, centrally concentrated morphology, with a subtle deviation from perfect elliptical symmetry, possibly indicating a mild tidal interaction. A slightly fainter and bluer knot is visible at the bottom end of the galaxy, which may signify a region of active star formation, possibly due to the aforementioned tidal interaction. No distinct spiral arm structures or dust lanes are readily apparent.
