The galaxy presents as a spiral type, exhibiting a prominent central bulge that appears moderately sized. The spiral arms are clearly defined, displaying a tightly wound structure that suggests a relatively older stellar population within the arms. The orientation is such that the galaxy is viewed at an angle, but not quite edge-on, permitting a clear view of the spiral structure. A noticeable bar feature extends through the center, contributing to the overall morphology. The galaxy's color profile indicates a mix of older, yellower stars in the bulge and potentially younger, bluer stars in the spiral arms, though detailed color gradients are subtle in this image. There may be some sign of disturbances with a slightly lopsided appearance. No obvious signs of a major merger are visible.
