The galaxy presents as a disk galaxy, viewed at an oblique angle, with a clear indication of a flattened structure. A prominent central bulge dominates the inner region, exhibiting a yellowish-white hue, suggesting an older stellar population. Fainter spiral arms emanate from the central bulge, tracing a relatively smooth, non-flocculent pattern. The outer disk appears bluer, indicating the presence of younger, hotter stars and ongoing star formation. The galaxy does not show significant signs of tidal disruption or major merger events. The disk appears moderately thick. A faint bar feature may be present in the central region, but it is not strongly pronounced. The galaxy exhibits a moderate amount of dust obscuration, particularly towards the outer regions of the disk. The overall morphology is consistent with an intermediate spiral type.
