The galaxy presents an elliptical morphology, appearing largely smooth and featureless. There is a concentrated central bulge exhibiting a yellowish hue, suggesting an older stellar population. The galaxy gradually fades into a diffuse halo extending outwards. There's no distinct evidence of spiral arms, dust lanes, or recent major merger activity within the resolution of the image. The color profile indicates a redder overall composition, which aligns with a low star formation rate. The shape of the galaxy is observed to be more elliptical than circular. There is a slight possibility of minor disturbances.
