This galaxy presents a generally smooth morphology with little discernible substructure. Its overall shape is approximately round, with only slight deviations from perfect circularity. The galaxy exhibits a color gradient, with the central region appearing more yellow, gradually transitioning towards a redder hue in the outer regions. This color distribution may indicate a central population of older stars and reduced ongoing star formation in the core, with younger, bluer stars being more prevalent in the outskirts. There is no strong evidence of spiral arms or a prominent bar structure. Indications of significant recent or ongoing major merger events or tidal disturbances are absent. There may be a slight asymmetry or minor disturbance detectable along the edge of the galaxy which could be a potential location of star formation. Overall, it appears to be a relatively evolved system with a well-defined spheroidal shape.
