The galaxy presents as an elliptical morphology, with a smooth, centrally concentrated light distribution. The core exhibits a yellowish hue, suggesting a population of older stars. A faint, extended halo surrounds the central region, displaying a subtle gradient from yellow at the core to a slightly bluer tinge in the outer regions. There is no obvious disk component or spiral arm structure. Indications suggest that it is not currently undergoing a major merger. Based on its appearance, it seems that the galaxy has a relatively low star formation rate.
