The galaxy presents as an elongated, elliptical-like structure. The light distribution is centrally concentrated with a bright, reddish core, suggesting an older stellar population. Moving outwards from the core, the light fades gradually, exhibiting a smoother texture with faint blue hues toward the edges. There is no distinct spiral arm structure or prominent dust lanes visible. The overall morphology suggests a galaxy that is relatively evolved, with a reduced rate of current star formation. The color gradient indicates possible ongoing, though limited, star formation activity in the outer regions. No significant morphological disturbances are apparent.
