The galaxy exhibits a generally smooth morphology, appearing as a flattened spheroid. A central bulge is present, exhibiting a yellowish hue, suggesting an older stellar population. Fainter, bluer light can be seen in the outer disk, suggestive of younger stars. The disk appears relatively undisturbed, although there may be a minor asymmetry to the upper left portion. There is little to no evidence of ongoing major merger activity or significant tidal disturbances, with the overall structure appearing settled. The galaxy displays an intermediate ellipticity, appearing neither perfectly round nor highly elongated.
