The galaxy presents a largely smooth morphology, with a highly concentrated central bulge. The overall shape appears approximately round, though there's a slight suggestion of ellipticity. Color gradients are observed; the core exhibits a yellow-gold hue, indicating an older stellar population likely dominated by evolved stars. The outer regions fade to a redder color suggesting the same older population. The absence of prominent spiral arm structures and dust lanes reinforces the characterization of this galaxy as relatively evolved, and having little ongoing star formation. Any faint disk presence, if it exists, is not easily discerned at this resolution. There are no obvious signs of tidal disturbances or ongoing major merger activity affecting the system's overall structure.
