The galaxy presents as a flattened spheroid, exhibiting a smooth, centralized concentration of light. A distinct nucleus is observed, appearing bright and nearly white. The galaxy lacks well-defined spiral arms or a prominent disk structure. The color gradient transitions from a bluer core region outwards to redder hues at the periphery. This suggests a mix of stellar populations, with potentially younger, hotter stars concentrated in the center and older, cooler stars dominating the outer regions. There is a very slight distortion in the shape, but the overall structure doesn't show major disturbances characteristic of recent merger events.
