The galaxy appears to be a lenticular or early-type spiral with a relatively smooth, featureless morphology. It presents a largely uniform, elliptical shape. The central bulge region is notably brighter than the surrounding disk, exhibiting a diffuse luminosity gradient outwards. There are hints of a very faint disk structure, but distinct spiral arms are not apparent. The light distribution suggests an older stellar population, with less evidence of ongoing active star formation. A slight distortion may be present in the disk, possibly indicative of a minor gravitational interaction or past merger event. The galaxy shows a redder color overall.
