The galaxy presents as a relatively smooth, elliptical-like structure. It has a bright, concentrated central bulge that graduates outward to a less defined, fainter halo. The galaxy exhibits a slight elongation, departing from perfect circularity. There is a hint of a disk, but it is not well defined. The overall color is yellowish, suggesting an older stellar population dominating the light output. There is no clear evidence of spiral arms or active star formation regions based on the color and morphological characteristics observed. No significant signs of tidal disturbances or recent merger activity can be observed.
