The galaxy exhibits a generally smooth morphology with a high degree of roundness. The central region presents a concentrated luminosity profile, indicating a prominent bulge component. The color gradient transitions from a yellowish-white core to a more reddish-orange periphery, suggesting a potential radial variation in stellar populations, with older, redder stars dominating the outer regions. The overall structure shows no evidence of significant spiral arms or a well-defined disk. There may be a very small amount of minor disturbance in the system, but it is largely undisturbed. There is a clear dominance of non-blue stars.