The galaxy presents a largely smooth, elliptical morphology. Its central region exhibits a bright, concentrated bulge with a yellowish hue, indicative of an older stellar population. The light gradually diffuses outward from the core, transitioning to a fainter, more diffuse halo. There appears to be a subtle blueish tint in the outer regions of the galaxy. There are no clearly defined spiral arms or distinct dust lanes visible in the image, suggesting this galaxy is largely devoid of significant ongoing star formation. The overall shape is somewhat elongated, leaning towards an elliptical classification rather than perfectly spherical. No significant tidal disturbances or signs of an ongoing merger are visually apparent in the galaxy's structure.
