The galaxy presents as a concentrated, elliptical-like form with a relatively smooth light distribution. Its core exhibits a yellowish hue, indicative of an older stellar population, with potentially diminished star formation activity. There is a subtle color gradient visible, transitioning to slightly bluer tones in the outer regions, hinting at the presence of some younger stars, but the color difference is minimal. The galaxy shows no obvious spiral arm structures or significant dust lanes and appears generally undisturbed. There are no major distortions or signs of ongoing merger activity discernible in the image. The galaxy appears moderately compact, and the overall shape is close to circular with only a slight elongation.
