The galaxy exhibits an elliptical morphology, appearing largely featureless and smooth in structure. It displays a concentrated central bulge that gradually diffuses into a less dense halo. The color profile suggests an older stellar population, indicated by the yellowish-red hue, more dominant toward the core. There is no apparent spiral arm structure or significant dust lane obscuration visible. The overall shape appears moderately round, with no significant tidal disturbances, tails, or clear signs of an ongoing major merger event. There may be signs of minor disturbances, but the galaxy appears largely undisturbed and relatively isolated.
