The galaxy presents as a spiral galaxy, observed at an angle that is not quite edge-on. The central bulge is moderately prominent, exhibiting a yellowish-white color, which suggests an older stellar population. Fainter spiral arms extend from the bulge, displaying a bluer hue indicating the presence of younger, hotter stars and ongoing star formation. No significant morphological disturbances are readily apparent. The spiral arms appear somewhat loosely wound. There is no distinct bar structure. Overall, the galaxy appears relatively isolated, with no signs of major interaction with other galaxies.
