The galaxy presents a generally smooth and rounded morphology. The central region exhibits a high degree of luminosity, suggesting a concentrated nucleus. While a disk structure appears to be present, it lacks sharply defined spiral arms. There are some subtle, but not well-defined disturbances in the galaxy shape, potentially indicating ongoing minor interactions or internal dynamics. Colors appear to be relatively consistent throughout the galaxy, with only slightly bluer hues noticeable in the outer disk regions, potentially indicating more recent star formation in those areas. The galaxy does not show obvious signs of a major merging event or significant tidal features.
