The galaxy presents with a moderately compact morphology, appearing relatively smooth. There is a notable color gradient across the galaxy's profile. One region appears to exhibit a bluer hue, suggesting the presence of younger stellar populations and possibly ongoing star formation. In contrast, another area shows a more yellow or reddish tint, potentially indicating older, redder stars or dust obscuration. The object exhibits signs of potential tidal interactions or merging activity. A plume or tail-like feature is suspected emanating from the main body, or may be a second object. The overall shape is somewhat elliptical but exhibits notable asymmetries.
