The galaxy presents as a moderately luminous object with an elongated, cigar-shaped morphology. Its color appears somewhat redder compared to field stars, indicating an older stellar population. The galaxy's structure is generally smooth, with little evidence of distinct spiral arms or significant dust lanes. The overall light distribution suggests a centrally concentrated mass. There is also a second galaxy slightly right of the first that appears smaller.

There may be signs of weak tidal features suggesting past or ongoing gravitational interaction with another galaxy. The shape of the galaxy could be due to one or more past mergers. Further spectroscopic analysis would be needed to confirm this.
