The galaxy presents as a somewhat elongated, cigar-shaped object with a smooth overall appearance. The color distribution suggests the presence of recent or ongoing star formation, with bluer hues dominating the central region, indicating the presence of hot, young stars. There are no obvious spiral arm structures or distinct features. The galaxy appears relatively isolated with no clear signs of tidal interactions or mergers, though there seems to be a minor asymmetry in the main body that could be from a previous interaction. It may be a disk galaxy with a low inclination angle.
