The galaxy presents a somewhat amorphous morphology, lacking a well-defined spiral arm structure or a prominent central bulge. It appears as a diffuse, extended object. There is evidence of internal structure, showing some slightly brighter regions that could potentially be areas of more intense star formation. The galaxy exhibits a mostly smooth appearance, yet there are indications of possible disturbances or interactions, given its subtle irregularities. Its color indices suggest it contains a mix of stellar populations, ranging from young, blue stars to older, redder stars, but the overall dominant color seems to be in the yellow/redder spectrum. The light is somewhat concentrated in the center, which might suggest a central nucleus, but it is not very well defined. Based on its appearance it might be undergoing some minor disturbances or interactions.
