The galaxy presents a somewhat amorphous appearance. There is a centrally concentrated bulge region that appears yellowish in color, possibly indicating an older stellar population. Surrounding this bulge, there's a disk or halo structure with a bluer hue, suggestive of younger stars and/or ongoing star formation. The disk shows some indications of disturbances, possibly due to minor interactions. Overall, the galaxy does not appear to have a well-defined spiral structure and has some non-negligible irregularities.
