The galaxy presents as a luminous, elliptical form. A central bulge is apparent, exhibiting a concentrated intensity that gradually diminishes towards the outer regions of the galaxy. The overall color profile suggests an older stellar population, with a yellowish hue dominating the bulge and inner regions. A subtle bluer component is visible in the outskirts, hinting at the presence of some younger, hotter stars in the galaxy's outer reaches. The galaxy exhibits a smooth texture. There is no strong evidence of prominent spiral arm structures or significant dust lanes. The observed ellipticity suggests a flattened spheroidal shape, but it does not resemble a disk galaxy. There are no signs of any major tidal disturbances or ongoing mergers.
