This galaxy presents as a spiral type, viewed at an oblique angle. The central bulge is moderately prominent and appears bright white, indicative of an older stellar population. Fainter spiral arms extend from the bulge, exhibiting a somewhat clumpy morphology. The arms appear bluer in color compared to the bulge, suggesting the presence of ongoing star formation. A faint bar structure may be present, bisecting the central bulge. The overall ellipticity of the galaxy is moderate, implying a noticeable, but not extreme, degree of flattening. There is no obvious sign of major disturbance or merging activity.
