The galaxy presents as an elliptical morphology, with a smooth and diffuse light distribution. The central region exhibits a concentrated, bright core, gradually fading towards the outer edges. The galaxy's color gradient displays a yellowish-orange hue in the core, potentially indicating an older stellar population. There appears to be no distinct spiral arm structure or significant dust lane obscuration. The overall shape is elongated, with the ratio of the major to minor axis suggesting an E4 or E5 classification on the Hubble sequence. There are no apparent tidal features, such as streams or shells, indicating no recent major merger events. The galaxy is approximately 8 kpc across, and roughly 35% the distance to the edge of the observable universe. The low star formation rate is consistent with a galaxy dominated by older stars.