The galaxy presents a generally smooth morphology, with a subtle elongation visible in its overall shape. The color profile suggests an older stellar population, with a dominant yellowish hue emanating from the central region. A slight color gradient can be observed, transitioning towards a somewhat bluer tinge in the outer regions, potentially indicating the presence of younger stars or ongoing star formation, though at a low rate. There appears to be no strong evidence of prominent spiral arms or a distinct disk-like structure. There is a suggestion of a tidal interaction. The structure is largely undisturbed.
