The galaxy presents as a centrally concentrated object with a generally smooth morphology. The core exhibits a bright, yellowish-white luminosity, suggesting a population of older stars. There is minimal evidence of spiral arm structure or dust lanes. A slightly elongated shape is observed, but the galaxy is mostly round. There is a faint diffuse halo surrounding the central region. A bluer region appears to the upper left, which could signify a region of active star formation, or a region of scattered light. There is no indication of a major ongoing merger event, though the presence of a minor disturbance is plausible given the slight asymmetry of the galaxy's halo.
