The galaxy appears to be a relatively smooth, disk-like structure, with a slightly elongated, cigar-like shape. There is a central bulge region that shows a yellowish hue, possibly indicating an older stellar population. Evidence of a disk is present with hints of bluer, possibly younger stars on the outer edges of the galaxy. There is no obvious presence of tidal tails or other features suggesting a recent major merger event, but some minor irregularities might be present suggesting a minor interaction or internal disturbance. There is a low overall star formation rate.
