This galaxy presents as a relatively compact structure, with an apparent diameter of roughly 20 arcseconds. The galaxy exhibits a relatively smooth morphology, with a distinct lack of spiral arm features or a prominent bulge. The color profile suggests a slightly higher concentration of redder stars towards what appears to be the galactic center, though this could be affected by dust attenuation. There are some faint irregularities present in the outer regions, which may indicate either minor tidal interactions with other galaxies or internal disturbances. No clear evidence of a recent major merger is apparent in this image, but a slight asymmetry in the outer profile is present.
