The galaxy presents as a relatively smooth, elongated structure. Its overall shape is somewhat cigar-shaped, with a bright, concentrated central region that likely corresponds to the galactic nucleus. The light distribution suggests it is a fairly elliptical galaxy.  There is a slight color gradient noticeable, with the central region appearing bluer and the outer regions exhibiting a redder hue. There is a lack of distinct spiral arms, which further suggests an older stellar population with less active star formation occurring in the galaxy, specifically the outer regions. The outskirts of the galaxy fade gradually into the background, with no sharp truncation or disruption that would indicate a recent major merger event. There are no noticeable dust lanes or patches within the galaxy. Some minor disturbances are possible, but the bulk of the galaxy's light is undisturbed.
