The galaxy presents as a relatively smooth, elliptical-like structure. There is a concentrated central bulge exhibiting a yellowish-white hue, suggesting an older stellar population. The galaxy appears to have a relatively homogeneous distribution of light, with no prominent spiral arm structures or dust lanes visible. There is potentially a faint, diffuse halo surrounding the central region, indicated by a subtle fading in intensity outwards from the core. The overall color profile suggests a mature galaxy with a moderate redshift. The light output appears to be from older, redder stars. There's a small redder region to the right, indicating a small pocket of younger or redder stars. The galaxy appears relatively isolated, showing no signs of significant tidal disruption or interaction with neighboring galaxies in this field of view.
