The galaxy presents an overall elliptical morphology with a smooth light distribution. The central bulge region exhibits a concentrated, bright yellowish-white glow, indicating a potentially older stellar population. Moving outward from the center, the galaxy displays a fainter, bluish halo extending beyond the central region, hinting at some ongoing or recent star formation activity. The lack of distinct spiral arms suggests a classification towards early-type galaxies, specifically an elliptical or lenticular type. The galaxy appears moderately inclined, with a noticeable elongation along one axis. There might be a slight warp or distortion visible in the outer regions, although subtle, possibly due to past interactions or internal dynamics.
