The galaxy appears to be an elliptical or lenticular galaxy, exhibiting a smooth, diffuse morphology with no discernible spiral arms or bar structure. It is characterized by a generally round shape. There is evidence of a potential ongoing merger or tidal interaction. It shows hints of disturbed morphology, with the galaxy possibly composed of two distinct luminosity peaks or an apparent uneven light distribution. The color gradient shows that the upper portion is slightly bluer, while the lower portion is reddish. This suggests a potential spatial variation in stellar population, with regions of more recent star formation in the bluer region and older, redder stellar populations dominating the reddish region. However, it's hard to determine exact features given the resolution. The galaxy is fairly massive, indicating a relatively high stellar mass content. Its star formation rate appears suppressed.