The galaxy presents as a well-defined spiral with a relatively small bulge. The spiral arms are tightly wound and somewhat patchy, suggesting active star formation regions. The color profile indicates a blue hue in the spiral arms, indicative of a younger stellar population. The overall morphology appears relatively undisturbed. There is no apparent bar structure within the central region. The galaxy exhibits a moderately high degree of central concentration. The apparent size of the galaxy appears moderate given its likely distance. There is no obvious tidal debris or significant interaction with any companion galaxies in the immediate vicinity, though some minor disturbance of the morphology of the galaxy can not be ruled out.
