The galaxy presents as a somewhat elongated structure with an approximate physical radius of 3.8 kpc. There is a prominent bulge, which has a smooth appearance. Faint spiral arms are present but ill-defined. The color gradients suggest ongoing or recent star formation, with regions of bluer light emanating from the arms, indicative of younger stellar populations. Some areas of redder light can be seen in the middle of the galaxy, potentially due to older stars or dust. The galaxy is overall relatively isolated, though a potential merging event cannot be ruled out.