This galaxy appears to be a spiral galaxy with a prominent central bulge. The bulge exhibits a smooth, concentrated morphology, with a bright, diffuse light distribution. The spiral arms are not sharply defined but can be traced outwards from the bulge, appearing somewhat flocculent and patchy. There is evidence of some ongoing star formation within the arms, indicated by the presence of bluer regions. The overall color of the galaxy is consistent with a mix of stellar populations, with a slightly redder bulge and bluer spiral arms. The disk appears to be relatively thin when viewed edge-on, with no substantial warp or asymmetry immediately visible. There are some faint traces of what could be minor tidal disturbances, but they do not appear to significantly disrupt the overall structure. The galaxy displays a moderate degree of central concentration, and the rate of star formation is relatively low.
