The galaxy presents as a roughly elliptical, concentrated object. Its core exhibits a high degree of luminosity. The colour profile suggests an older stellar population dominates, exhibiting a yellow-orange hue centrally, with a slight gradient towards redder colours in the surrounding areas. Indications of possible ongoing or recent merger activity are seen in its shape, suggesting a recent or current galaxy interaction event. Possible tidal tail features can be seen, though are very faint. The morphological features of the galaxy suggest it is largely smooth in structure, with little evidence of strong spiral arm features or significant dust lanes. The overall appearance indicates a relatively mature galaxy.
