The galaxy presents as a relatively smooth, elliptical structure with a concentrated central bulge. The galaxy's color is generally yellowish-white, suggestive of an older stellar population. It exhibits a moderate degree of roundness and a subtle change in luminosity from the core to the outer regions. There is no apparent evidence of significant spiral arm structure or ongoing major merger activity. The overall appearance indicates a relatively evolved galaxy with a quiescent star formation rate, possibly transitioning towards a red and dead state. A possible minor interaction or disturbance cannot be fully ruled out given the slight irregularities in the galaxy's outer halo.
