The galaxy presents a generally smooth morphology, with a high degree of central concentration of light. The overall shape appears to be relatively round. There is no discernible spiral arm structure or prominent disk features visible. Color gradients suggest a slightly yellower central region, potentially indicating an older stellar population in the galactic nucleus. No evidence of tidal tails, bridges, or strong morphological disturbances is apparent, suggesting that the galaxy is not currently undergoing a major merging event. There may be some faint underlying structure but the resolution is too low to make definitive statements about it. 
