The galaxy presents as a somewhat diffuse object, exhibiting a dominant central bulge. The bulge region displays a yellowish hue, suggestive of an older stellar population. There is a subtle disk component surrounding the bulge. The overall shape appears to be somewhat in between round and elongated. There are disturbances in the outer regions of this galaxy, suggestive of a possible interaction with another galaxy or recent merger activity. The disturbance can be described as minor.
