The galaxy presents a generally smooth morphology, though there are some features present indicating possible disturbances. It appears as a centrally concentrated mass of stars, with a fairly round overall shape. The light profile suggests some ongoing star formation activity, with slightly bluer hues detectable in the central regions. The relatively high luminosity suggests the presence of a significant stellar population. Possible merging activity is hinted at through slight distortions in the shape and some visible tidal tails, indicating past interactions with another galaxy. There also appears to be minor disturbances throughout the disk. Overall, the galaxy appears to be in the process of transformation.
