This galaxy appears to be a relatively smooth, elliptical galaxy with a concentrated central bulge. The light distribution suggests an elliptical shape, with the core region exhibiting a bright, yellowish hue, indicative of an older stellar population. There is a faint suggestion of a disk-like structure but it is not well defined. No distinct spiral arms or prominent dust lanes are visible. The galaxy appears relatively isolated, with no signs of major mergers or significant tidal disturbances. The morphology is consistent with a galaxy that has largely completed its star formation, with little ongoing star formation implied by the lack of blue color. The overall appearance suggests a dynamically relaxed system with a dominant spheroidal component.
