The galaxy presents a discernible spiral structure, exhibiting two prominent spiral arms that emanate from a central bulge. The arms display a moderate winding, neither tightly coiled nor loosely extended. Patches of bluer light can be seen along the arms, indicating regions of active star formation. The bulge appears relatively moderate in size, with a yellowish hue suggesting an older stellar population. The overall disk inclination is such that the galaxy is viewed at a slight angle, but not edge-on, allowing the spiral structure to be clearly observed. There is no strong evidence of a central bar structure. The galaxy does not appear to be undergoing a major merger or significant tidal disturbance, though some asymmetry may be present.
