The galaxy appears to be a spiral type, viewed at an oblique angle, but not quite edge-on. There is a noticeable central bulge that appears moderately sized relative to the disk. Spiral arms are discernible, though not sharply defined. A bar structure is present and appears to be prominent. The disk exhibits variations in color, with a slight bluer tint outside the central bulge, indicating recent star formation. The galaxy appears largely undisturbed, with no obvious signs of major merging activity, though minor disturbances could be present, but are not clearly visible. The overall morphology suggests a relatively evolved spiral galaxy with ongoing star formation.
