The galaxy presents as a relatively compact object, approximately 6.8 kpc in radius. Morphologically, it appears to be in the process of merging with one or more other galaxies, displaying significant tidal disturbances and asymmetries in its light distribution. A primary core is evident, surrounded by fainter, elongated structures that suggest ongoing gravitational interactions. The overall color suggests a mixed stellar population, with areas of both older, redder stars and regions of more recent star formation that appear bluer in color. The galaxy has a prominent blue central region, which might indicate higher levels of star formation. Despite the presence of star-forming regions, the smoothness of a portion of the galaxy suggests that it is also undergoing significant amounts of transformation due to the ongoing interactions.
