The galaxy presents a discernible disk structure, viewed at a slight angle relative to edge-on. Its shape is somewhat elongated, appearing roughly elliptical. The galaxy exhibits spiral arm morphology, with predominantly loose windings. A significant portion of the disk shows evidence of active star formation regions, indicated by the presence of localized blue concentrations. The central bulge region appears relatively small and not overly prominent in comparison to the overall disk size. The spiral arm count seems to be primarily two, with an uncertainty regarding the exact number due to the image resolution. There is morphological evidence suggesting a possible minor disturbance or interaction, potentially indicating a past or ongoing merger event. The overall color profile leans toward the bluer side, suggestive of a substantial population of young, hot stars.
