The galaxy appears to be composed of two main components: a larger, more diffuse structure and a smaller, more concentrated region. The larger component exhibits a smooth morphology, potentially an elliptical galaxy seen at an angle. Its light is shifted toward the red end of the spectrum, indicating an older stellar population, with the overall shape appearing elongated and cigar-shaped.

The smaller component is characterized by a bluer color, suggestive of ongoing star formation activity. This bluer region is more compact and less uniformly shaped than the larger component. This galaxy is estimated to have a moderate stellar mass. There are no obvious signs of major mergers, although minor disturbances might be present.
