The galaxy presents as a relatively smooth, elongated structure. It displays a central bulge exhibiting a slightly reddish hue, potentially indicating an older stellar population. Extending outwards from the bulge are fainter, disk-like features, with hints of bluer color, possibly suggesting ongoing star formation. The overall morphology appears somewhat cigar-shaped, lacking a clearly defined spiral structure. There are no obvious signs of a major merger event or significant tidal disturbances. The galaxy shows no distinct features, such as prominent dust lanes or bright star-forming regions. The disk blends smoothly into the surrounding space.
