The galaxy presents a morphology that appears predominantly smooth, with a hint of a disk-like structure. It appears to be an elliptical galaxy. The colour profile displays a concentration of redder hues in the central region, indicative of an older stellar population, with bluer components appearing towards the periphery. There are subtle irregularities and a faint disturbance, suggesting possible interactions with minor disturbances from other galaxies, although the central region is largely undisturbed. The overall shape appears generally elliptical with the galaxy being in an intermediate state with it neither being completely round or elongated. Star formation activity appears to be suppressed to a low level, with a relatively low rate of new stars forming, evidenced by the overall older stellar population suggested by the redder colour and a small indication of some blue colour. The galaxy's mass appears to be significant, corresponding to a substantial stellar mass.
