The galaxy presents as a single, relatively smooth object with a concentrated central bulge. The morphology is generally elliptical, exhibiting a high degree of roundness in its overall form.  The central region displays a yellowish hue, potentially indicating an older stellar population or significant dust extinction.  There is faint evidence of a very subtle disk or perhaps a faint feature extending from the core. No signs of a major ongoing merger are immediately apparent, though a very minor disturbance is possible, perhaps a faint tidal tail or asymmetry. The color gradients suggest a relatively evolved system, though some ongoing star formation cannot be ruled out.
