The galaxy presents as a relatively small, faint, and somewhat diffuse object. Its morphology appears to be primarily smooth, suggesting a classification towards the elliptical or lenticular end of the Hubble sequence. However, there is a subtle hint of disk-like structure and some irregularity, possibly indicating minor disturbances or ongoing interactions. The galaxy's color is a muted blue-white, implying a moderate population of young, hot stars, though star formation activity seems relatively low overall. There is no obvious central bulge or spiral arm structure visible. The object is not perfectly symmetrical, with some indication of tidal features or asymmetries. The image quality makes precise classification challenging, but it seems to lie between a smooth elliptical and a disturbed disk galaxy.
