The galaxy presents as a relatively small, somewhat elongated structure. Its overall color appears to be composed of primarily older stellar populations, emitting light that shifts towards the redder end of the spectrum. The galaxy exhibits a generally smooth morphology, lacking prominent spiral arms or a distinct central bulge. There are hints of some subtle features, such as a possible faint disk or a very minor irregularity in its shape, which would suggest there is a more recent or ongoing interaction. The galaxy's light is not perfectly circular. It exhibits a noticeable degree of ellipticity, indicating it is not viewed perfectly face-on.
