The galaxy appears as a centrally concentrated object with a smooth, elliptical morphology. Its light profile suggests a relatively featureless structure, lacking prominent spiral arms or a well-defined disk. The galaxy exhibits a color gradient, appearing slightly bluer in its outer regions and transitioning to a more yellow/red hue towards the center. This color variation could imply older stellar populations dominating the core, with younger, bluer stars present in the outer regions. There's a subtle asymmetry in the galaxy's outer isophotes, potentially indicative of a minor gravitational interaction or past merger event that has not completely disrupted the overall structure. The size of the galaxy appears moderate, suggesting it is an intermediate-mass system, neither a dwarf galaxy nor a massive elliptical.
