The galaxy presents as a centrally concentrated object with a smooth morphology. There is a notable lack of well-defined spiral arms or a prominent disk structure. The central region exhibits a yellowish hue, possibly indicative of an older stellar population. Moving outward from the core, the color transitions to a slightly bluer tint, which may reflect the presence of younger stars. This blue light component seems fairly subdued. There may be low level star formation occurring throughout the galaxy. Overall, the galaxy appears to be relatively undisturbed, lacking any obvious signs of ongoing major mergers or significant tidal disruptions. Its structure suggests a system that has likely evolved through secular processes. 
