The galaxy presents a morphology consistent with a spiral type, though with some noticeable peculiarities. It is not viewed edge-on; the disk appears at an angle. Prominent spiral arm structures are visible, exhibiting a somewhat flocculent nature, without grand design characteristics.

The central bulge is moderately sized, though it does not appear to be the dominant feature of the galaxy. A bar structure appears to be present but is not particularly strong or well-defined.

There is an apparent distortion within the structure that implies a possible interaction or merger event. It is not a full merger, but a disturbance suggesting a minor interaction or a possible ongoing accretion event. The disk appears to be in good shape though, the bulge is mostly undisturbed, and it does not resemble a classical merger.

The overall light distribution suggests a substantial population of both older and younger stars. The presence of bluer regions within the arms and the more yellowish hue of the central bulge support this.
