The galaxy presents as a primarily smooth, elliptical-like structure with a concentrated central bulge exhibiting a yellowish hue, suggestive of an older stellar population. There is some asymmetry, with a hint of disk-like or spiral features that are slightly bluer, perhaps indicating regions of more recent star formation or a more complex morphology than a pure elliptical galaxy. The galaxy appears to be relatively isolated. There may be signs of a minor gravitational disturbance or interaction.
