The galaxy presents a moderately elliptical morphology. Its core exhibits a concentrated, yellowish-white light, suggesting a population of older stars. A diffuse, greenish halo surrounds the core, potentially indicating ongoing, albeit low, levels of star formation. The halo is not uniformly distributed, showing a slight elongation, possibly indicative of tidal interactions or an early stage merger. Patches of reddish light are interspersed, possibly areas of dust obscuration or localized star formation. The overall appearance is that of a relatively smooth galaxy, with only subtle signs of morphological disturbances.
