The galaxy presents as a generally smooth, elliptical morphology, with a moderately round appearance. The central bulge exhibits a concentrated luminosity, suggesting a high stellar density. The color gradient transitions from a yellowish-white core to a slightly bluer periphery, possibly indicative of a radial variation in stellar populations or dust content. There is a suggestion of a faint disk-like structure. There does not appear to be any significant signs of tidal disturbances or ongoing major merging events. The overall structure suggests a mature galaxy with limited current star formation activity.
