The galaxy presents a generally smooth, elliptical morphology, appearing mostly featureless at this resolution. The central region exhibits a brighter, more concentrated light profile, suggesting a prominent bulge. Moving outwards, the light gradually fades, and there is evidence of a faint, diffuse disk or halo surrounding the central bulge. There is a hint of bluer hues in the outer regions, suggestive of possible younger stellar populations compared to the core. The overall structure indicates that this is likely a relatively massive galaxy with minimal ongoing star formation. There are no visible signs of tidal disturbances or interactions with other galaxies, indicating a relatively isolated system.
