The galaxy presents as a somewhat elongated, smooth structure. It is dominated by a central bulge exhibiting a yellowish-orange hue, suggesting an older stellar population within. This central region appears relatively uniform in color and luminosity. Fainter, bluer patches are observed on the lower left side, which could indicate regions of more recent star formation. The overall shape is more in between a round and cigar shaped galaxy. While there are not clear signs of ongoing major mergers, there might be minor tidal disturbance due to the slight irregularity of the outer regions of the galaxy. The main body of the galaxy has a fairly consistent luminosity gradient.
