The galaxy presents as a single, relatively smooth object with a centrally concentrated luminosity profile. It appears elliptical, with a high degree of roundness. The color gradient suggests an older stellar population, with a yellowish hue dominating the central region, potentially indicating the presence of evolved stars. There is little indication of significant ongoing star formation or distinct spiral arm structures in the visible bands. Faint blue edges indicate little to no star formation. The absence of any notable tidal features or morphological disturbances indicates that the galaxy does not appear to be undergoing any major mergers or significant gravitational interactions with other galaxies at this time.
