The galaxy presents as an elliptical morphology, appearing largely smooth in texture with a highly concentrated central bulge. Its color profile suggests an older stellar population, exhibiting a yellowish-red hue, indicative of evolved stars and a reduced rate of ongoing star formation. The galaxy displays a moderate degree of ellipticity, appearing more elongated than perfectly circular. There is no discernible evidence of spiral arm structures or significant dust lanes. There appears to be no major ongoing merger events, the galaxy shows no strong tidal tails or irregular shapes. There is a hint of possible minor disturbances in the galaxy's outer regions, but these are not prominent.