The galaxy presents as a slightly elongated, disk-like structure oriented at an oblique angle relative to the observer's line of sight. The central region appears relatively smooth and concentrated, exhibiting a yellowish-orange hue. This may indicate an older stellar population within the bulge. The outer regions of the galaxy show a hint of disk-like structure, with some suggestion of spiral arm morphology, though the resolution is limited. These arms appear bluer in color compared to the central region, possibly indicating ongoing star formation. There are no obvious signs of a major ongoing merger event. However, subtle asymmetries or minor disturbances are not entirely ruled out. The galaxy has a generally smooth appearance.
