The galaxy presents a generally smooth morphology, appearing largely featureless in the available imagery. Its shape is moderately elliptical, trending toward being rounded rather than elongated. The galaxy's color profile indicates a redder overall hue, suggesting a population of older stars. There are faint hints of some internal structure that may suggest the presence of a disk. There is no strong evidence of ongoing merging activity, though subtle asymmetries could point to minor gravitational interactions. Given the estimated redshift of 0.158281, this is a relatively distant galaxy.