The galaxy presents as a relatively smooth, centrally concentrated object with a slight elongation, appearing somewhere between round and cigar-shaped. It exhibits a dominant bulge component that is yellowish-white in color. There is a faint hint of bluer light in the outer regions, potentially indicating some level of ongoing star formation, with an estimated star formation rate greater than one solar mass per year. Evident distortion suggests that the galaxy may be undergoing some sort of interaction or disturbance, possibly with a minor or major merging event.
