The galaxy presents as a flattened spheroid with a bright, concentrated central bulge. The light from the bulge appears relatively smooth, lacking any distinct features. The surrounding disk exhibits a gradual fading of luminosity from the center outward. There is some mottled texture, and a slight bluer hue on one side of the galaxy, indicating potential star formation. There are no strong indications of spiral arm structure, although this could be due to resolution or viewing angle. There appear to be some possible signs of tidal disturbance on one side, but a higher quality image would be necessary for verification. Based on these observations, the galaxy appears to be a transitional disk galaxy with possible ongoing interactions with other galaxies.
