The galaxy presents a generally elongated, cigar-shaped morphology. The central region displays a high concentration of luminosity, appearing bright and yellowish. The light becomes more diffuse and blueish towards the outer edges, suggesting the presence of a stellar disk component. While there appears to be a disk, the image lacks a distinct spiral structure. There is no obvious evidence of ongoing major mergers or significant tidal disturbances. The galaxy appears to be a relatively isolated system in a late stage of its evolution, as evidenced by the high fraction of light that is smooth with little features.
