The galaxy presents as a centrally concentrated, spheroidal object with a smooth light distribution. The core exhibits a bright, yellowish hue, suggesting a significant population of older stars. The color gradually fades to a redder tone in the outer regions of the galaxy, also consistent with an aging stellar population. No distinct spiral arm structures or prominent dust lanes are discernible. The overall morphology indicates an elliptical galaxy, potentially of type E4-E5, based on its apparent ellipticity. There is no apparent evidence of ongoing major merger activity or significant tidal disturbances, though faint asymmetries at the limits of the visible structure cannot be entirely ruled out. The galaxy is relatively massive and displays low star formation.
