The galaxy presents as a relatively smooth, centrally concentrated object. Its morphology is generally elliptical, exhibiting a high degree of sphericity. The light distribution appears quite uniform, lacking prominent spiral arms or strong bar features. There is a slight elongation but this does not deviate much from round. Colour gradients appear minimal across the galaxy's extent. The galaxy's surface brightness is moderately high, with no significant signs of active star formation regions visible at this resolution. There are very subtle indications of some disturbances in the galaxy's outer regions but the overall system appears to be relatively isolated and dynamically relaxed.
