The galaxy presents a generally smooth and elliptical morphology. It appears to be moderately elongated in shape. There is a central concentration of light that fades gradually towards the edges, consistent with a spheroidal distribution of stars. A slight blueish tint can be observed in the outer regions, possibly indicating ongoing, but relatively low levels of star formation. There is no clear evidence of spiral arm structure or significant dust lanes. The overall appearance suggests a relatively mature stellar population. There appears to be no significant signs of recent major merger activity, or any obvious tidal features present. Minor disturbances may be present, but cannot be definitively determined. The galaxy is not perfectly round, but instead appears to be more "in between" round and cigar-shaped.
