The galaxy presents as a relatively smooth, elliptical form, approximately 9 kpc across. The central region exhibits a high concentration of light, appearing significantly brighter and yellower than the outer regions, hinting at an older stellar population. The outer regions diffuse gradually, showing a lower surface brightness and a slight color shift towards redder hues. There is no clear evidence of spiral arms or a distinct disk. The galaxy shows only minor disturbances, no signs of an ongoing major merger, and only very weak indications of tidal interactions. Its overall shape appears to be largely spheroidal, with the luminous material symmetrically distributed around a well-defined center. Based on its color and shape, this galaxy appears to be a massive, evolved system.
