The galaxy appears as a moderately bright, slightly elongated object with a predominantly smooth morphology. There is little evidence of distinct spiral arms or a prominent bar structure. The galaxy's color is a relatively uniform yellowish-white, suggesting a stellar population that is not dominated by very young, blue stars, although ongoing star formation cannot be ruled out. It appears to be relatively isolated, with no obvious signs of a major ongoing merger or tidal interactions with other galaxies. It is most likely an elliptical or lenticular galaxy, given the smooth appearance, but a face-on spiral galaxy with faint arms could also be possible. It has a size that is relatively large compared to the neighboring objects in the field. There is a slight asymmetry in the light distribution, which could be caused by the beginnings of a minor merger.
