The galaxy presents a generally smooth morphology, lacking prominent spiral arms or a distinct disk structure. It appears largely spheroidal in shape, exhibiting high degree of central concentration. The galaxy's color profile suggests a dominant population of older stars, indicated by the yellow to reddish hue of its central region. The outer regions exhibit a bluer tint, potentially indicating the presence of younger stellar populations or ongoing star formation. There are indications of very mild disturbances. The galaxy does not appear to be undergoing any major merging events, and the overall structure suggests a relatively relaxed and evolved system.
