The galaxy presents as a relatively smooth, elongated object. Its morphology suggests an elliptical galaxy, viewed at an oblique angle. The central region exhibits a concentration of light with a yellowish-orange hue, indicating an older stellar population. Moving outward from the core, there is a subtle transition towards a blueish color, potentially indicating the presence of some younger stars, although the overall blue fraction appears low. The galaxy's shape appears more cigar-like than round, with no obvious spiral arms or strong indications of a disk structure. There appears to be a slight disturbance within the outer regions of the galaxy, but it is unclear whether there are any signs of a major ongoing merger.
