The galaxy presents as a somewhat elliptical structure, elongated along a diagonal axis. The light distribution is centrally concentrated with a smooth profile, suggesting an older stellar population is dominant. There are no prominent spiral arms or dust lanes visible, indicating a lack of significant ongoing star formation. The galaxy's color appears generally redder, which is consistent with a population of older, cooler stars. There may be slight irregularities in the outer edges, hinting at possible past interactions or minor disturbances to its morphology. The general appearance suggests a galaxy that is likely nearing the end of its star-forming activity and evolving toward a more quiescent state.
