The galaxy presents as a moderately bright, yellowish-white object with a somewhat smooth morphology. There are no strong indications of spiral arms or a well-defined disk structure. The light distribution appears relatively uniform throughout the galaxy's body, though with slight concentrations in the central region, indicating a possible nucleus. Based on its smooth appearance, it is likely an elliptical galaxy. The object exhibits a degree of roundness. There is no clear evidence of ongoing mergers or major disturbances, though a slight asymmetry to the light distribution might suggest a minor interaction in its past. The galaxy's colour suggests a population of older stars with limited ongoing star formation activity.
