The galaxy exhibits a smooth, elliptical morphology. It possesses a bright, concentrated nucleus, indicative of a significant stellar population density within the central region. The color appears to be a yellowish-white, suggesting a population of older stars with lower star formation activity. There is little evidence of spiral arms or a well-defined disk structure. The galaxy presents a generally rounded shape, lacking any strong elongation or asymmetry. There is no clear indication of ongoing major mergers or significant tidal disturbances. The overall appearance suggests a galaxy that has largely completed its morphological evolution, with a dominant spheroidal component and minimal recent star formation.
