The galaxy presents as a relatively compact object. It appears to have an overall smooth morphology, though there is evidence of interaction or merging activity occurring. Two distinct components are observed. The larger of the two, in the upper left quadrant, is bluish in color, possibly indicating a population of younger, hotter stars. The second component appears more reddish-orange and is located to the right of the brighter area, indicating an older stellar population. A faint plume is observed emanating outward from the galaxy, toward the lower half, which could indicate a tidal tail caused by gravitational interaction.
