The galaxy presents as a moderately inclined spiral system. The central bulge appears relatively smooth and concentrated, with an elongated shape suggesting a potential bar structure. Faint spiral arms emerge from the bulge, exhibiting a patchy distribution of star formation regions, indicated by slight color variations within the arms. The overall color suggests a galaxy populated by both older stellar populations and ongoing star formation. The galaxy exhibits no strong signs of tidal disturbances or interactions with other galaxies, implying it is a relatively isolated system.
