The galaxy presents as a generally smooth object with an elliptical morphology, though some slight irregularities can be observed. The color profile indicates a predominantly evolved stellar population. A bright, concentrated central bulge dominates the luminosity. The overall roundness of the galaxy suggests it is likely an elliptical galaxy, viewed at an angle that does not clearly show any disk-like features. There is a faint hint of disk, but not so pronounced. No evidence of major merging events or tidal tails can be seen. There is a hint of disruption to the surrounding galactic light.
