The galaxy appears to be relatively compact, exhibiting an approximate diameter of ~7 arcseconds. It has a slightly irregular morphology. There is a dominant central bulge that appears fairly luminous.

There is some evidence of a disk structure. While the disk is not sharply defined, there is a more diffuse, less luminous area surrounding the bulge, extending outward. The galaxy's color profile suggests varying stellar populations. The central bulge exhibits a more yellow/red hue, while the surrounding disk shows some bluer colors. This may indicate a mix of older stars in the center and younger, star-forming regions in the disk. 

There is also some indication of minor tidal disturbances or possible merging activity. A slight asymmetry is observed in the galaxy's outer regions, which could be caused by gravitational interactions. The presence of these features warrants further investigation to confirm the galaxy's evolutionary state.
