The galaxy presents as a relatively smooth, elliptical structure. It exhibits a concentrated central bulge that transitions smoothly into a fainter, more diffuse halo. The core displays a yellowish hue, suggesting an older stellar population. There's no clear evidence of spiral arms or significant dust lanes within the disk, reinforcing its classification as an elliptical galaxy. The galaxy's overall color appears redder, which implies that star formation is either minimal or has ceased. It appears as an isolated galaxy, as no other galaxies are around it to disturb its shape. The morphology hints at a relatively evolved system, possibly experiencing little to no recent merger activity.
