The galaxy presents as a somewhat elliptical structure with a prominent, concentrated central bulge. The core exhibits a yellowish-orange hue, suggesting an older stellar population likely dominated by evolved stars. Fainter, bluer light extends outward from the central bulge, indicating a less concentrated, more dispersed disk component with ongoing, but relatively low, levels of star formation. The disk appears relatively smooth, without prominent spiral arms or significant dust lanes visible at this resolution. The galaxy shows a slight asymmetry, with some diffuse light extending more noticeably on one side, possibly indicating a past or ongoing minor interaction. The overall color suggests a galaxy with a considerable mass in stars and a relatively low specific star formation rate, implying a galaxy that has largely ceased active star formation.
