The galaxy appears as a relatively compact, centrally concentrated object. Its overall form suggests an elliptical morphology, potentially exhibiting a slight deviation from perfect circularity. The light profile appears smooth, lacking prominent spiral arms or a well-defined disk structure. The dominant color is bluish, indicating the presence of a younger stellar population and ongoing star formation. A faint, diffuse halo is visible surrounding the central body of the galaxy, extending outwards. There are no strong indicators of any major tidal disruptions or ongoing mergers, though subtle asymmetries might indicate minor disturbances. 
