The galaxy presents as a relatively smooth, centrally concentrated structure, likely an elliptical galaxy. It exhibits a noticeable color gradient, transitioning from a bright, yellowish-white core to a fainter, slightly redder halo. There is no clear evidence of spiral arms or a distinct disk component. The galaxy appears somewhat elongated but is not excessively cigar-shaped. No significant signs of tidal disturbances or ongoing major merger activity are apparent, though minor irregularities cannot be ruled out at this resolution. The smooth texture and color profile suggest an older stellar population and relatively low levels of current star formation.
