The galaxy presents as a smooth, somewhat elongated structure, lacking any readily discernible spiral arms or a prominent central bulge. Its light distribution appears concentrated, fading gradually towards the outer edges. There is a subtle color gradient, with a slightly bluer core transitioning to a redder halo. No signs of tidal disturbances, merging events, or distinct features are observed in the available image. The overall morphology is indicative of an elliptical or lenticular galaxy, with a relatively high degree of central light concentration and an absence of strong star-forming regions within the limits of this image's resolution.
