The galaxy presents as a spiral galaxy viewed nearly edge-on from our perspective. There is a central bulge appearing somewhat large and prominent, with a generally rounded morphology. A flattened disk extends outwards from either side of this bulge. The disk's dust lanes are indistinct, but there is some mottled detail visible indicating some structure. There is a generally smooth texture to the disk, appearing to be consistent in nature along its length.

The colors present suggest a mixture of stellar populations. The bulge appears more yellowish, possibly indicating older stars, while the disk seems more greenish. This could be due to the presence of younger, hotter stars and ongoing star formation within the disk. There does not appear to be evidence of any significant tidal disturbances or a major merger event. There is a slight suggestion of a possible minor companion or disturbance, but that may not be the case. The image suggests this galaxy is in a relatively undisturbed state.
