The galaxy presents as a single, largely featureless object. It exhibits a generally elliptical morphology, appearing more rounded than elongated. A smooth, centrally concentrated light distribution dominates the galaxy's appearance. There is a gradual decrease in luminosity from the core outwards, with no distinct spiral arms, bars, or rings visible. The galaxy appears a yellow-white hue, which suggests an older stellar population, although there may be some regions of active, ongoing star formation. There are no obvious signs of recent or ongoing major mergers, though some minor irregularities in the outer regions may indicate past interactions.
