The galaxy appears as a relatively smooth, centrally concentrated object. It exhibits an elliptical morphology with a predominantly round shape. There is no clear evidence of spiral arm structure or a prominent disk. The galaxy's light profile suggests a relatively old stellar population, although there may be some ongoing, low-level star formation. No major mergers or significant tidal disturbances are immediately apparent; however, subtle features may be present upon closer inspection. The galaxy displays a radial color gradient, becoming slightly bluer towards the outer regions, implying a change in the stellar population or dust content with radius.
