The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. The color profile indicates a significant population of older stars, exhibiting a yellowish hue towards the core. There is minimal evidence of spiral arms or prominent dust lanes. A faint, diffuse halo surrounds the galaxy. The overall morphology suggests a system undergoing or having completed its transition to a more passive, quiescent state of star formation. No major disturbances are visible in the image, suggesting a period of relative isolation or stability.
