The galaxy presents as a spiral, albeit with a dominant, bright central bulge. The spiral arms are not sharply defined, instead appearing somewhat diffuse and flocculent. There is an overall smoothness to the light distribution, suggesting a relatively evolved stellar population. The galaxy appears more rounded than elongated, but not perfectly circular.

Evidence of interaction is minimal; no significant tidal tails or distorted morphology are readily apparent, although some minor irregularities in the spiral arm structure could indicate past or ongoing interactions. The overall impression is of a relatively undisturbed galaxy, likely with ongoing, but perhaps not particularly vigorous, star formation within the disk. The yellow-red color suggests the presence of older stars.
