The galaxy presents as a centrally concentrated object with a largely smooth appearance. Its shape is approximately round, with only a slight deviation from perfect circularity. The central region is bright and has a blue-white color, suggesting ongoing star formation. There is evidence of some disturbance within the galaxy, possibly indicating a past minor merger or tidal interaction. However, no major ongoing merging activity is apparent. The estimated mass of the galaxy appears to be on the lower end, suggesting a relatively smaller galaxy with a lower star formation rate.
