The galaxy presents as a largely smooth, elliptical structure. It exhibits a concentrated central bulge with a significant amount of light emission, likely indicating a high density of stars in the core. The overall color appears to be dominated by redder wavelengths, suggesting an older stellar population with a lower rate of star formation. While generally elliptical, there is a slight deviation from perfect roundness, leaning towards an intermediate shape. No distinct spiral arms or major disturbances from mergers are visually apparent; however, there may be a faint indication of a minor interaction or tidal feature in the galaxy's outskirts. The galaxy is well-defined with a moderate degree of central concentration.
