The galaxy presents a morphology consistent with an elliptical galaxy, appearing largely featureless and smooth in overall structure. The central region exhibits a bright, concentrated core. A gradual decline in luminosity is observed moving outward from the center, indicating a centrally concentrated stellar population. The galaxy's color suggests an older stellar population, the redder hues likely indicating a dominance of evolved stars. There are no obvious spiral arms or dust lanes visible. The shape appears to be close to circular, with only slight elongation. There is a possible minor asymmetry in the outer regions, hinting at a potential past interaction. The galaxy is a significant distance away, so finer details are not discernible. 
