The galaxy presents as an elliptical or lenticular structure, appearing largely smooth and somewhat elongated. Its central region exhibits a high concentration of light, suggesting the presence of an older stellar population or a possible supermassive black hole. There's a subtle color gradient from the central region to the outer regions, shifting from yellowish-white towards a slightly bluer hue, hinting at ongoing, albeit subdued, star formation within its disk or outer regions. Faint hints of what might be spiral arm structures are seen in the outskirts. There's a slight asymmetry in the outer isophotes, potentially indicative of a minor gravitational interaction or merger event in its past. No significant dust lanes or prominent star-forming regions are immediately apparent.
