The galaxy presents a generally smooth and rounded morphology. The primary body of the galaxy exhibits a dominant red-shifted color profile, likely indicative of an older stellar population and/or significant dust obscuration. A fainter secondary component, located at a slight offset, shows bluer hues, suggesting the presence of younger, hotter stars, indicating a possible region of active star formation. There appears to be little evidence of strong tidal features or prominent spiral arm structures. The overall appearance suggests an elliptical galaxy or a lenticular galaxy with minimal features. The galaxy shows no signs of a major ongoing merger, though some minor gravitational disturbance cannot be ruled out.
