The galaxy presents as a single, relatively smooth object with a predominantly elliptical morphology. There is little to no visible disk structure or spiral arm features evident. The galaxy exhibits a concentrated central bulge region which appears bright and yellowish, suggesting an older stellar population. The galaxy appears to be generally spheroidal in shape, exhibiting a high degree of roundness. No signs of tidal tails, strong gravitational lensing effects, or any other major disturbances indicative of recent or ongoing merger activity are apparent in this image. The color gradient of the galaxy suggests possible variations in stellar population or dust distribution, with a gradual shift toward a more reddish hue in the outer regions.
