The galaxy presents as a single, relatively smooth, and concentrated light source. It appears approximately elliptical in shape, with a degree of roundness. There is a lack of distinct spiral arm structure or prominent features suggestive of a disk. The galaxy exhibits a yellowish-white hue, indicative of a population of older stars. There is no sign of ongoing major merger activity or significant tidal disturbances, though a minor disturbance cannot be ruled out. The galaxy appears isolated, without any obvious companion galaxies or significant interaction.
