The galaxy presents as a spiral type, observed at an inclination that allows for detailed examination of its structure. Two prominent spiral arms emanate from a central region, exhibiting a loose winding pattern. The arms are well-defined and possess a clumpy morphology, suggestive of active star formation regions along their lengths.

The central region, while visible, does not exhibit a pronounced bulge. A subtle, elongated structure, possibly a weak bar, appears to traverse the center. The overall color of the galaxy indicates a relatively high star formation rate. The arms show a bluer hue, indicative of younger, hotter stars, while the central region appears slightly redder, potentially hosting an older stellar population. There is evidence of a recent merger or interaction, as tidal tails are visible. The galaxy appears asymmetrical, suggesting a dynamic and potentially unstable structure.
