The galaxy presents a smooth, elliptical morphology. Its core exhibits a concentrated, bright luminosity, suggestive of an older stellar population. The galaxy shows a slight elongation, with the shorter axis approximately 80% of the length of the longer axis. The overall color profile appears to be relatively uniform across the galaxy, trending towards redder wavelengths, which further indicates an older stellar population with limited recent star formation. There are no signs of significant spiral arm structures, dust lanes, or tidal features that would indicate recent mergers or interactions. The galaxy's profile decreases smoothly in intensity from the center outwards, with no prominent substructures visible in this imaging.
