The galaxy appears to be a single, relatively isolated object. It exhibits an elongated, cigar-shaped morphology. The galaxy's light profile seems largely smooth, indicating a lack of strong spiral arm structures or prominent dust lanes. The central region appears slightly brighter and yellowish in color, suggesting an older stellar population. The outer regions are less well-defined, with a subtle gradient in brightness. There is no visible evidence of a major ongoing merger event, although there is some subtle irregularity in the outer region.
