The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. A subtle color gradient is observed, shifting from a bluer hue at the core to slightly redder tones in the outer regions. No distinct spiral arm structures or prominent dust lanes are visible. There is an apparent lack of significant morphological disturbances, such as tidal tails or obvious signs of an ongoing major merger. The galaxy appears relatively isolated, with no immediate companion galaxies detected in close proximity. Its overall appearance suggests a relatively evolved system, potentially an elliptical galaxy with a modest amount of ongoing star formation.
