The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. A gradual fading of luminosity extends outward from the core, suggesting a spheroidal morphology. There are hints of a possible extended, faint disc structure but the image resolution makes this uncertain. The color profile is generally redder in the central bulge and shifts slightly bluer moving outwards. There are small, blueish regions, possibly young star forming regions within the galaxy. The galaxy appears somewhat rounded, however, there is asymmetry in the outer regions, suggesting a possible past or ongoing minor gravitational interaction or merger. The overall structure does not suggest a major ongoing merger.
