The galaxy appears as a centrally concentrated, elliptical-like object with a relatively smooth light distribution. It exhibits a pale bluish-white coloration, suggesting a population of younger, hotter stars and potential ongoing star formation. The shape is slightly elongated, showing a moderate ellipticity but with an aspect ratio close to unity. There is no visible spiral structure or prominent disk. The outer regions appear fainter and more diffuse. The object lacks any signs of significant disturbances like tidal tails or strong asymmetries, indicating that the galaxy is most likely not undergoing a major merger event, although minor interactions cannot be ruled out.
