The galaxy presents as a relatively smooth, centrally concentrated object with a near-circular morphology. There is minimal evidence of distinct spiral arms or a prominent bar structure. The central region exhibits a bright, compact core indicative of a concentrated stellar population. The light profile gradually diminishes from the core outwards. There is a slight bluish hue in the central region, possibly indicating ongoing star formation. No signs of major merging or tidal disturbances are apparent. The galaxy is not perfectly elliptical but shows a slight deviation from a perfect circle. There might be minor disturbances that can't be seen with this resolution.
