The galaxy presents as a well-defined elliptical or lenticular structure with a smooth, diffuse appearance. The central region exhibits a concentration of light, indicative of a bulge, with a color gradient shifting towards warmer hues. The outer regions of the galaxy appear bluer, potentially reflecting the presence of a younger stellar population or ongoing star formation. The overall shape is elongated, with a clear major and minor axis, but the lack of distinct spiral arms or prominent dust lanes suggests that it is not a spiral galaxy. There does not appear to be any signs of tidal disturbances or mergers in the image.
