The galaxy presents as a moderately sized, elliptical or lenticular structure, exhibiting a smooth, diffuse light distribution. A slight elongation is observed, deviating from a perfectly circular morphology. The light profile shows a concentration towards the central region, with a gradual decrease in intensity towards the outer edges. The overall color appears reddish-yellow, suggesting an older stellar population with minimal recent star formation. No distinct spiral arms or dust lanes are discernible. There is evidence of possible minor tidal disturbances in the form of faint asymmetries or extensions, suggesting previous interactions or mergers.