The galaxy presents as a primarily smooth, elliptical structure, characterized by a concentrated central bulge. It exhibits a generally rounded morphology, though not perfectly circular. The color profile suggests a largely older stellar population, with a noticeable concentration of light in the yellow-red spectrum, particularly towards the galactic center. This indicates a region dominated by evolved stars. There is a faint hint of bluer light in the outer regions of the galaxy, possibly signifying the presence of some younger, star-forming regions. However, star formation appears to be subdued in the galaxy as a whole. There is no obvious evidence of spiral arm structure. Finally, the galaxy's overall symmetry does not show any substantial disturbances that may point to tidal interactions or a merging event.
