The galaxy presents as a dominant, centrally concentrated object with a smooth overall appearance. It exhibits a roughly elliptical morphology, appearing somewhat rounded in shape, with only subtle deviations from a perfect ellipse. There may be some minor disturbances in the morphology. The galaxy's core is noticeably brighter than its outer regions, indicating a relatively high concentration of stellar mass toward the center. Color gradients are subtle, though the central region appears slightly redder than the outer disk. This might suggest an older stellar population at the core compared to the outer regions. Star formation is occurring at a relatively low rate. Although there's no clear indication of a major ongoing merger event, closer examination reveals hints of minor disturbances or possible interactions, suggesting past or ongoing gravitational interactions with another galaxy.
