This galaxy presents a largely smooth morphology, with minimal discernible features. The light distribution suggests a central concentration of older stars, as indicated by the yellowish hue towards the center. Progressing outwards, the galaxy transitions to bluer tones, hinting at younger stellar populations in the outer regions, with moderate star formation activity. Its shape is neither perfectly spherical nor significantly elongated, rather in between. There is no evident sign of a major merger, but possible minor disturbance in structure. Overall, this galaxy appears to be a mature system, potentially a disk galaxy viewed at an angle.
