The galaxy presents as a relatively compact structure. Its morphology is largely smooth, with some subtle features suggestive of a possible disk-like component although lacking well-defined spiral arms. The color profile indicates a generally redder population, but has some blue regions. There might be minor disturbances or tidal features implying some interaction with neighboring galaxies. It appears that the galaxy is neither actively merging, nor undisturbed. The intermediate roundness hints it is in between round and elliptical.
