The galaxy presents as a relatively smooth, centrally concentrated object, exhibiting an elliptical morphology. The light profile appears to decrease monotonically from the core outward, with no readily discernible spiral arm structure or distinct features. There is a slight elongation, deviating from a perfectly circular shape. The color profile is generally consistent with an older stellar population, exhibiting a redder hue, although a hint of bluer light may be present in the outer regions. No significant tidal features or signs of recent major mergers are immediately apparent, although a subtle asymmetry could suggest minor disturbances. The overall appearance is suggestive of a mature galaxy with a dominant spheroidal component.
