This galaxy exhibits a generally smooth morphology, with a high degree of roundness. There appears to be a concentrated central bulge region exhibiting a pale red/yellow hue, which is consistent with a population of older stars. Fainter bluish halos appear to surround this region. The galaxy does not present any obvious signs of significant ongoing merging activity or major disturbances. The object appears to be relatively compact. Given the color distribution, the inferred star formation rate is seemingly low.
