This galaxy appears to be a relatively smooth, elliptical or lenticular galaxy. It exhibits a central concentration of light, with a generally featureless disk. The overall color suggests a population of older stars, leaning towards redder wavelengths. The lack of prominent spiral arms or dust lanes reinforces its classification as an early-type galaxy. There might be faint, subtle disturbances in the outer regions, possibly indicative of a past minor merger event, although the main body of the galaxy shows no major distortion. The galaxy is elongated, not perfectly circular, with a mostly uniform color gradient throughout the disk. There may be some weak star formation, but this is likely quite low.
