The galaxy presents as a fairly smooth object, ellipsoidal in shape, with a noticeable elongation. It displays a dominant central bulge region that is a yellowish-orange hue, suggestive of an older stellar population. The disk component is less defined but appears to exhibit some bluer, less prominent regions, hinting at more recent star formation, particularly at the edges. There is no strong evidence of spiral arm structure or a bar feature. Faint hints of dust lanes are present. The galaxy exhibits no signs of a major merger or significant tidal disturbances.
