The galaxy presents as a relatively compact, luminous object with a smooth appearance. It is elongated in shape, exhibiting a moderate ellipticity. The color profile suggests a dominant stellar population. The central region displays a brighter intensity, potentially indicative of a concentrated nucleus or bulge component. There appears to be some interaction occuring. One side seems more distorted, with a more compact companion. The galaxy exhibits a smooth luminosity gradient from the core outwards, suggesting little in the way of spiral arms or large scale star formation.
