The galaxy presents as an elliptical or lenticular morphology, exhibiting a central bulge with a smooth luminosity profile. There is a lack of strong spiral arm structure. The galaxy appears slightly elongated. The central region shows a yellow-white hue, suggesting an older stellar population. Fainter, bluer light is subtly present in the outer regions, hinting at some ongoing or recent star formation, though it is not extensive. The edges of the galaxy appear diffuse, lacking a sharp boundary. Minor disturbances or interactions with other objects cannot be ruled out, but there is no strong evidence of a major merger event.
