The galaxy exhibits a moderately bright core, appearing nearly spherical in overall morphology. The light distribution appears relatively smooth, with a subtle radial gradient in intensity moving outward from the central region. No distinct spiral arm structures are discernible. There may be faint, diffuse extensions, or tidal tails, hinting at potential past interaction, but these are ambiguous. The galaxy presents a color gradient, with bluer hues in the outer regions suggestive of younger stellar populations. A slight asymmetry in its overall light distribution could also be indicative of minor disturbances. There is an indication that it is primarily non-merging, but I would want to gather more evidence.