The galaxy presents a predominantly smooth morphology, with a hint of a feature or disk-like structure. The overall shape is tending towards round, with a slight deviation toward an intermediate form. The light distribution appears concentrated towards the center, suggesting a prominent bulge. There is a possibility of a minor interaction or disturbance, considering the fuzziness and asymmetry in its outermost regions. The galaxy has a yellowish hue, indicating a possible lack of significant ongoing star formation and a population dominated by older stars. However, the presence of some bluer regions suggests that some star formation activity is still present. Overall, the galaxy appears to be a relatively massive system, possibly undergoing a merger.
