The galaxy presents as a concentrated, centrally-brightened object. Its overall morphology is somewhat smooth, with a subtle extension or disturbance visible in the outer regions. The core appears spheroidal and displays a yellowish-orange hue, potentially indicating an older stellar population. Fainter, bluer colors in the surrounding halo suggest the presence of some younger stars or active star formation, although this activity seems relatively subdued. The galaxy does not appear to be undergoing any major merging events, though a slight asymmetry in the outer regions could indicate a minor interaction or disturbance. 
