The galaxy presents as a lenticular, cigar-shaped structure, exhibiting a relatively smooth morphology. Its color indices suggest a higher emission in the redder bands, which could indicate an older stellar population. There is no pronounced disk structure visible; instead, the light distribution appears centrally concentrated with a gradual decrease in intensity towards the outer regions. It shows no obvious signs of significant ongoing merging activity or major disturbances; however, a slight asymmetry or irregularity in the light distribution might suggest a possible minor interaction in its recent past. The overall characteristics point towards a passively evolving system with a high stellar mass, but a low star formation rate.
