The galaxy presents as a spiral galaxy with a moderately sized bulge relative to its disk. The spiral arms are tightly wound. Two dominant spiral arms are clearly visible. The core of the bulge exhibits a yellowish hue, suggestive of an older stellar population. The spiral arms display a bluer coloration, indicating the presence of younger, hotter stars and ongoing star formation. There appears to be no significant bar structure visible. Overall, the galaxy appears relatively undisturbed, without evidence of a major ongoing merger, though minor disturbances cannot be ruled out.
