The galaxy presents an overall elongated, cigar-shaped morphology, suggesting it may be either an elliptical galaxy or a spiral galaxy viewed edge-on. The central region exhibits a concentrated, bright core, likely indicative of a bulge component. The galaxy appears relatively smooth, lacking prominent spiral arms or other distinct features typically observed in disk galaxies. However, faint hints of asymmetry or possible tidal features are present at the edges of the galaxy, suggesting a possible past interaction with another galaxy. The color profile indicates that the central region is more yellow or white, potentially indicating an older stellar population. The outer regions of the galaxy appear slightly bluer, implying the presence of younger stars or ongoing star formation, albeit at a low rate. The galaxy is relatively small, implying a low mass. 
