The galaxy presents as an elongated, cigar-shaped structure with a smooth, relatively featureless morphology. Its color appears to be predominantly redder, suggesting an older stellar population with potentially lower rates of recent star formation. There is no clearly discernible spiral structure or disk-like appearance. A subtle color gradient seems to exist across the galaxy's body, with the central region exhibiting a slightly more intense red hue compared to the edges. There are indications of minor morphological disturbances, but these are not overly prominent, implying that any interactions or mergers are not presently of a major, disruptive nature. Based on this, it likely resides at a considerable distance.
