The galaxy presents as an elliptical morphology, exhibiting a generally smooth appearance without prominent spiral arms or a well-defined disk structure. There is an observed elongation, presenting as an oval shape, suggesting it is not perfectly spherical. The central region demonstrates a higher concentration of light, appearing bright and yellowish-gold in color, likely indicating a substantial population of older stars. A faint greenish hue is visible within the surrounding halo, possibly indicative of ongoing, but minimal, star formation, or a population of younger, hotter stars. The galaxy displays potential signs of minor disturbances, such as asymmetry in its outer regions. Overall, the galaxy appears to be a massive system undergoing a quiescent phase of stellar formation.
