The galaxy presents as a moderately luminous, relatively compact object. Its overall appearance is smooth and elliptical, lacking any distinct spiral arm structures or prominent features. The color appears to be concentrated toward the redder end of the spectrum, which suggests an older stellar population with fewer young, hot stars. There may be minimal dust obscuration in the field of view. The galaxy does not appear to be undergoing any major interactions or exhibiting signs of significant disturbances or ongoing merger events. The object's shape is roughly circular. 
