This galaxy appears to be an elliptical type, exhibiting a smooth, centrally concentrated morphology. There is little evidence of a prominent disk structure or spiral arms. The light distribution suggests a high degree of symmetry, being largely devoid of significant asymmetries or irregularities. 

The galaxy displays a yellowish-white hue towards the center, with the color gradually shifting towards slightly bluer tones in the outer regions. This color gradient may indicate differing stellar populations, with older, redder stars concentrated in the core and younger, bluer stars distributed more sparsely in the outskirts. No obvious signs of recent or ongoing major mergers are apparent, though the outer regions may hint at minor tidal disturbances or interactions.
