The galaxy presents a largely smooth morphology with a concentrated central region. Its overall shape appears elliptical, though not perfectly rounded, exhibiting a slight elongation. The core displays a yellowish-orange hue, suggesting a population of older stars. Surrounding the core, the galaxy's outer regions exhibit a faint greenish tint, possibly indicating some level of ongoing star formation, albeit limited. There is no clear evidence of spiral arms or a well-defined disk structure. The galaxy doesn't appear to be undergoing any major merging activity, though there might be a minor disturbance visible in its outer halo. Overall, the galaxy appears to be a relatively massive system with an estimated stellar mass above 10^11 solar masses, currently exhibiting a low star formation rate.
