The galaxy presents a generally smooth appearance, with some suggestion of a disk-like structure. The central bulge is prominent and exhibits a yellow-orange hue, possibly indicative of an older stellar population. The surrounding disk appears less defined, with hints of blue suggesting the presence of younger stars. The galaxy appears somewhat elongated, but is mostly rounded. There is no obvious sign of a major ongoing merger, though some minor irregularities or faint tidal features might be present.