The galaxy presents as a lenticular or early-type spiral galaxy, viewed at a significant inclination. A distinct bulge component exhibits a yellowish hue, indicating an older stellar population. The disk, while present, appears relatively smooth and featureless, with a subtle bluish tint suggesting the presence of some younger stars. 

Evidence suggests a possible minor interaction or disturbance affecting the galactic structure; a secondary, fainter patch of light appears slightly offset from the main body, potentially indicating tidal debris or a smaller interacting galaxy. Overall, the galaxy appears to be in a relatively quiescent state, but the subtle structural irregularity hints at past or ongoing gravitational interaction with another system.
