The galaxy presents as a centrally concentrated system, appearing largely smooth in morphology. The light distribution suggests an elliptical or lenticular galaxy type. The core region appears bright, gradually decreasing in luminosity towards the outer regions. There is no clear evidence of spiral arms or a distinct disk. The galaxy exhibits a somewhat rounded shape, though a subtle elongation may be present. No major disturbances or merging events are clearly visible, though a very slight asymmetry is apparent in the outermost regions. The galaxy appears to be relatively isolated. The overall color is consistent with a population of older stars, indicating relatively low star formation.
