The galaxy presents as an elliptical or lenticular type, exhibiting a generally smooth, centrally concentrated morphology. The light distribution suggests a bulge component that dominates the galaxy's overall appearance. There is a slight elongation, transitioning it to a more cigar shape, but it is still fairly symmetrical. The color gradient indicates a population of older stars and potentially a dearth of ongoing star formation. The light is reddish with small hints of blue on the edges. There is no apparent spiral arm structure or significant dust lane obscuration, although resolution limitations impede detailed assessment of internal features. No large-scale tidal features or signs of recent major mergers are evident, implying relative isolation.
