The galaxy presents as a somewhat centrally condensed object with a relatively smooth light distribution. There is a slight elongation visible, deviating from a perfectly circular shape. The core region exhibits a brighter, more intense luminosity, suggesting a higher density of stars or potentially an active galactic nucleus. The overall color appears to be bluish, indicative of a younger stellar population and ongoing star formation, though a precise spectral analysis would be needed to confirm this. Faint, disturbed features are visible around the galaxy. These might be tidal tails or streams, indicating a possible interaction or merger with another galaxy in the past.
