The galaxy presents as a relatively smooth, elliptical-like structure, characterized by a high degree of central concentration. The core exhibits a bright, yellowish-white luminosity, suggesting a population of older stars. There is a subtle color gradient, transitioning from the yellowish core to a slightly redder hue in the outer regions. No distinct spiral arms or bar features are discernible, suggesting either an elliptical morphology or a face-on spiral with very tightly wound arms beyond our detection capabilities. The object does not appear to be undergoing a major merger or strong tidal interaction, although minor irregularities or faint features within the extended halo cannot be entirely ruled out at this resolution. Overall, the galaxy appears relatively quiescent with a low star formation rate.
