The galaxy presents with a central, bright core region surrounded by a more diffuse halo. The overall shape approximates a slightly elongated spheroid. The central core exhibits a bluish-white color, suggesting the presence of relatively young, hot stars or significant ongoing star formation activity. The outer halo appears more greenish in tone, potentially indicating a population of older stars or emission from ionized gas. There is some evidence of possible tidal disturbances or faint extensions, though this is not definitively clear. The galaxy does not show a clear spiral structure or prominent disk features. 
