The galaxy presents as a primarily smooth object, exhibiting a high degree of central concentration. Its morphology appears elliptical, though slightly elongated, trending towards an "in between" shape rather than perfectly round or cigar-shaped. There are no apparent major disturbances or signs of ongoing merging events, though minor disturbances cannot be completely ruled out. The galaxy emits strongly in the g, r, and z bands, with magnitudes relatively similar, suggesting a consistent spectral energy distribution across these wavelengths. This spectral characteristic may be indicative of a population of older stars. Based on its red color, the galaxy likely contains a large population of older stars. This would be consistent with a relatively low star formation rate. The effective radius of the galaxy is estimated to be on the order of several kiloparsecs.
