The galaxy presents as a flattened ellipsoid, exhibiting a smooth, rather than flocculent, texture across its visible surface. Its color profile is suggestive of an evolved stellar population, displaying a concentration of yellow and red hues towards the central bulge, indicative of older, cooler stars. Fainter blue tinges are visible in the outer disc regions, implying that some amount of star formation is still occuring, though at a low rate. No prominent spiral arm structure or other distinct features are immediately apparent. There appears to be little to no dust obscuration within the galaxy. The general morphology suggests a lenticular, or possibly an elliptical, type galaxy viewed at an angle. There is no obvious evidence of a recent or ongoing major merger event based on visible distortions or tidal tails. There is no obvious nearby galaxy interacting with this one.
