The galaxy presents as a roughly elliptical shape, although there is some suggestion of a slight disk structure. The central region exhibits a bright, concentrated luminosity, suggesting a prominent galactic nucleus. The light distribution appears relatively smooth, with a lack of pronounced spiral arm structures or prominent dust lanes. The color profile appears to show a bluer hue in the outer regions with more red in the center. There is some very slight evidence of tidal disturbance, or perhaps a recent minor merger, but generally the galaxy appears relatively undisturbed. Overall, the galaxy appears to be a galaxy between a spiral and an elliptical, perhaps a lenticular or a late stage spiral.
