The galaxy presents as a relatively compact object with a smooth, concentrated light profile, potentially exhibiting characteristics of an elliptical or lenticular morphology. The primary color is a yellowish-orange hue, suggestive of an older stellar population with a relatively low rate of ongoing star formation. There is evidence of a possible tidal disturbance or merger event. There appear to be two central objects, potentially galactic nuclei, and the galaxy appears elongated, with an irregular overall shape that might be attributed to gravitational interactions. The galaxy does not display prominent spiral arm structures or well-defined features typically associated with actively star-forming regions.
