The galaxy presents a generally smooth morphology, with a dominant central bulge exhibiting a somewhat elongated, cigar-like shape. While a distinct disk structure is not immediately apparent, there are subtle hints of features that disrupt the overall smoothness of the galaxy, with what looks like a possible minor disturbance. The galaxy's color profile appears relatively uniform, with no prominent color gradients that would suggest significant differences in stellar populations across its structure. It exhibits what seems like a very low rate of star formation.
