The galaxy presents a largely smooth and rounded morphology, with minimal discernible substructure at this resolution. The galaxy exhibits a centrally concentrated luminosity profile, appearing brightest at its core, with the light intensity gradually decreasing outwards. The color is a yellowish-white, suggesting a stellar population dominated by older, evolved stars. The absence of prominent spiral arms or significant dust lanes indicates that this galaxy is likely an elliptical galaxy, possibly in a relatively quiescent state, with little ongoing star formation. There are no obvious signs of tidal disturbances or mergers, with a seemingly undisturbed structure. The overall appearance suggests a relatively evolved and stable system.
