This galaxy presents an elongated, cigar-like morphology. There appears to be a primary body, showing a relatively smooth light distribution with a blue tint. A smaller, distinct component can be observed nearby, suggesting a potential interaction or a satellite galaxy. The blue color suggests ongoing or recent star formation within at least portions of the galaxy, although its rate is comparatively low. It is difficult to confirm if it has spiral arms or a disk-like structure due to the limited resolution, but it is possible that the galaxy has a disk component. The smooth light distribution suggests the possibility of features being obscured by dust or being a result of the viewing angle. There may be some evidence of minor tidal disturbances, possibly hinting at past or ongoing interactions with other galaxies.
