The galaxy presents as a spiral type, exhibiting a generally flattened disk structure viewed at a slight angle. The central bulge appears moderately prominent, displaying a yellowish-white hue which may indicate an older stellar population and minimal ongoing star formation in that region. Spiral arms are discernible, although somewhat flocculent and not tightly wound. The arms show hints of blue, suggesting the presence of younger, hotter stars, and thus active star formation. A subtle bar-like structure may be present across the galaxy's core, though not particularly pronounced. There appears to be some minor disturbance in the galaxy's morphology, possibly hinting at gravitational interaction with another galaxy at some point, or internal instabilities.
