The galaxy presents as a spiral, with a prominent disk structure. Two main spiral arms emanate from the central bulge, exhibiting a well-defined winding pattern that appears to be of intermediate tightness. The bulge itself is relatively pronounced, with an apparent size suggesting it contributes significantly to the overall luminosity. The galaxy's color profile indicates a mix of stellar populations, the central bulge appears more yellow/red, potentially indicating an older population, while the spiral arms show a bluer tinge, hinting at ongoing star formation. There is no indication of any major ongoing merger, but some minor morphological disturbances might be present within the disk structure. The galaxy appears to be a barred spiral.
