The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a somewhat elliptical morphology, appearing mostly round but not perfectly so. There is a suggestion of a diffuse halo surrounding the brighter central region, although the faintness and extent of this feature are difficult to ascertain with certainty. The color profile indicates a possible presence of older stellar populations, based on its redder hue, but there is still some star formation occurring as evidenced by slight blue color in the central region. There's no obvious evidence of spiral arms, bars, or major tidal disturbances in this image, suggesting the absence of a recent major merger event, though minor disturbances are not ruled out.
