This galaxy exhibits a predominantly smooth morphology with a hint of a disk structure. It appears to be a relatively undisturbed system, lacking any obvious signs of a major merger event. The galaxy presents an elongated shape, suggesting an edge-on or highly inclined orientation with respect to our line of sight. There is a slight color gradient, with the central region appearing somewhat more yellowish than the outer regions, potentially indicating a difference in stellar population or dust content. The outer regions have a soft, diffuse glow, while the central region appears more concentrated.
