The galaxy presents a generally smooth morphology, appearing largely spheroidal in shape. There is a concentrated central bulge that is more luminous, potentially indicating a higher density of stars. The galaxy exhibits a radial color gradient, transitioning from a yellowish core to a bluer outer region. This suggests that the outer regions may contain a population of younger, hotter stars, or that dust is obscuring redder light more effectively in those regions.

No distinct spiral arms or a clear disk structure are visible in the image. The object does not appear to be undergoing any major merger events or experiencing any significant tidal disturbances, with only a slight asymmetry visible. The image suggests it is a relatively isolated galaxy.