The galaxy presents a generally smooth morphology with a noticeable central bulge. While not perfectly spherical, the overall shape leans towards round, with a very subtle elongation. There's a hint of a disk-like structure but it's subtle and more suggested by color variation than distinct structural features. 

The galaxy's color gradient transitions from a warmer, yellowish hue at the core, potentially indicating an older stellar population, to cooler, bluer tones in the outer regions. This color variation may signify ongoing star formation in the outer regions of the galaxy, although the resolution limits a definitive identification of star-forming regions. There's no immediately obvious evidence of a recent major merger or significant tidal disturbances, but there may be slight asymmetry.
