The galaxy presents as a relatively smooth, elliptical structure with a high degree of central concentration. The core region exhibits a bright, yellowish-white hue, indicating a population of older stars. A faint, bluish halo surrounds the central bulge, potentially indicative of some ongoing, but limited, star formation in the outer regions. The galaxy appears elongated, with an approximate axis ratio of 3:1, classifying it as an elliptical galaxy of type E5 or E6 on the Hubble sequence. There is no visible evidence of spiral arms, dust lanes, or significant tidal disturbances suggesting a quiescent system without recent major merger activity. Faint, diffuse light extends beyond the main body, suggesting a relatively large stellar halo.
