The galaxy appears to be an elliptical galaxy, exhibiting a generally smooth and centrally concentrated light distribution. Its morphology is largely spheroidal, with a high degree of symmetry. There is little evidence of spiral arm structure or significant dust lanes. The central region is notably brighter and more compact than the outer regions. A smooth falloff of luminosity extending outwards suggests a fairly large radius. The color appears to be shifted toward the redder end of the spectrum, which could indicate an older stellar population and a lower rate of star formation. There may be a very slight elongation, but overall, the shape is close to circular. There is no obvious signs of interaction or recent merger events. The galaxy appears largely undisturbed.
