The galaxy presents as a spiral galaxy, exhibiting a defined disk structure, potentially with spiral arms, though resolution limitations prevent detailed tracing. A prominent central bulge is present, and appears to be moderate in size relative to the overall disk. Light distribution suggests the presence of a weak bar feature. There is evidence of a minor disturbance or interaction that could suggest a potential recent or ongoing merger event. The galaxy exhibits a bluer hue in certain regions, indicative of star formation, while overall color indices suggest a mixed stellar population. The galaxy is not seen edge-on.
