The galaxy presents as a largely featureless, elliptical-like object with a smooth, concentrated light profile. The core exhibits a bright, yellowish hue, suggesting an older stellar population. The outer regions fade gradually into the background sky, indicating a lack of distinct spiral arms or prominent dust lanes. The overall morphology implies a relatively evolved system with a high degree of radial symmetry. There is a very slight potential that it could have a disk, but it would not be well defined. Based on the color profile, it is likely a galaxy that is no longer very actively forming stars.
