The observed galaxy presents a discernible disk structure. It is face-on relative to our line of sight. The nucleus is distinctly bright, with a bulge that appears moderate in size. Faint spiral arms are observed emanating from the central region, though they exhibit a somewhat patchy and fragmented structure, they appear to be somewhat tightly wound. The galaxy exhibits an overall blueish color, suggesting the presence of ongoing star formation. No signs of any major disturbances or mergers are readily apparent. The galaxy appears as an isolated system.
