This galaxy presents as a single, consolidated object with a predominantly smooth morphology. The core exhibits a high degree of luminosity, appearing bright yellow-white, suggesting a concentration of older stellar populations. This luminosity decreases gradually toward the outer regions. 

No distinct spiral arm structures or prominent dust lanes are discernible. The overall shape of the galaxy is generally circular, with a lack of obvious distortions or tidal features, indicating a relatively relaxed system. There is no evidence of a recent or ongoing major merger event. Subtle irregularities or minor disturbances may be present in the outermost regions, but this is difficult to ascertain due to the limitations of image resolution. The color gradient suggests possible differences in stellar populations between the central bulge and outer halo, with bluer colors (potentially indicating ongoing star formation) appearing faintly in the periphery. The object does not show any apparent bar structure.
