The galaxy presents as a spiral type, exhibiting a prominent disk structure. Two distinct spiral arms are evident, winding moderately around the central bulge. The bulge appears relatively small compared to the overall size of the disk. The galaxy is slightly inclined relative to the observer's line of sight. The color gradients suggest active star formation regions within the spiral arms, imparting a bluer hue to these areas, with a general magnitude of about 17.3, whereas the bulge region exhibits a more yellowish-reddish, and possibly older stellar population. There is no major disturbance in the morphology, indicating that there is no current or very recent merger event. There may be a faint bar-like structure at the center of the bulge. The disk is quite extended and thin.