The galaxy presents as a relatively smooth, elliptical morphology with a concentrated central bulge. There is a slight elongation, but the overall shape is generally rounded. The color gradient transitions from a yellowish-white core to a bluer outer halo, suggesting a possible difference in stellar populations, with older, redder stars dominating the core and younger, bluer stars more prevalent in the outer regions. The galaxy shows no prominent spiral arm structures or obvious signs of major disturbances, and appears to be relatively isolated. Faint, diffuse extensions are present in the outer regions, potentially indicating tidal features or ongoing minor mergers. Overall, this galaxy appears to be an early-type system with a moderately high mass and a low rate of star formation.
