The galaxy presents as a relatively smooth, elliptical-like structure with a bright, concentrated central bulge. There is little evidence of spiral arms or a distinct disk component based on the image. The galaxy exhibits a color gradient, transitioning from a reddish-yellow core to a fainter, bluer outer halo. This suggests a possible variation in stellar population, with older, redder stars concentrated in the central bulge and younger, bluer stars in the outer regions, though star formation appears to be overall subdued. The galaxy's shape is moderately elongated, not perfectly spherical. There is some subtle indication of minor irregularities or disturbances in the outer regions, potentially suggesting past interactions or mergers, but no strong evidence of ongoing major merging activity is observed. Overall, this galaxy appears to be a quiescent, evolved system.
