The observed galaxy presents as a spiral type, exhibiting a prominent central bulge. The bulge appears moderate in size and exhibits a yellowish hue, indicative of an older stellar population. Two or three well-defined spiral arms emanate from the central bulge, which are relatively tightly wound. These spiral arms are bluer in color compared to the bulge, which is suggestive of ongoing star formation. A bar-like structure extends through the center of the bulge. The disk of the galaxy is oriented roughly face-on and extends beyond the spiral arms in a hazy manner. There appears to be no signs of major disturbances, such as tidal tails or significant asymmetries, suggesting that the galaxy is not currently undergoing a major merger.
