The galaxy presents as a relatively smooth, elliptical morphology. It is centrally concentrated, with the intensity of light gradually decreasing with distance from the center. The core exhibits a bright, yellowish-white hue, suggesting a population of older stars dominating the central region. There is a slight hint of redder colors extending further out from the core. No distinct spiral arm structure is visible, and the overall impression is one of a well-mixed, homogenous stellar population. The galaxy appears to be fairly isolated with no obvious signs of recent merger activity, tidal tails, or other strong gravitational interactions. The round shape implies the galaxy is likely viewed face-on.
