The galaxy presents as a relatively compact object with a smooth, largely featureless morphology. Its shape appears to be generally round, exhibiting minimal deviation from a circular form. The light is fairly uniform across the body of the galaxy, with some areas appearing somewhat brighter than others. There are no apparent spiral arm structures or a prominent central bulge. The color profile suggests a population of older stars. Evident is minimal dust obscuration, with the galaxy exhibiting a fairly uniform spectral signature across its entirety. There is no evidence of any tidal tails or strong gravitational interactions with other galaxies. The galaxy appears to be largely undisturbed, displaying a consistent structure throughout.
