The observed galaxy presents a generally smooth morphology. The central region appears bright and concentrated with a yellow hue, suggesting an older stellar population and minimal dust obscuration. Two regions of green emission are present on either side of the central bulge, and the round shape suggests a late-type, potentially lenticular, classification. There is an apparent lack of spiral arm structure, and a smooth and even light profile. The asymmetry and possible distorted structure of the galaxy suggests minor disturbances and possible past or ongoing interactions or tidal effects.
