The galaxy appears to be a relatively smooth, elongated structure, exhibiting a morphology suggestive of an elliptical or lenticular galaxy viewed at a significant angle. A bright, concentrated central bulge is visible, surrounded by a more diffuse, extended halo. Color gradients are present, with the central bulge displaying a yellowish-orange hue, indicative of an older stellar population. The outer regions of the galaxy appear bluer, potentially indicating the presence of younger stars, or a different stellar composition. There is no obvious evidence of spiral arms or significant dust lanes. The overall smoothness of the light distribution supports classification towards the early end of the Hubble sequence, likely an E or S0 galaxy. It does not appear to be undergoing any major merging events or exhibiting strong tidal disturbances. The galaxy is likely massive, though the present image lacks the resolution to resolve any distinct structures in the outer halo. The low star formation rate suggests a passive galaxy with limited ongoing star formation.
