The galaxy presents as a moderately luminous, elongated system with a smooth, featureless appearance, and a slight red-orange hue to it's core. Its morphology suggests an elliptical classification or perhaps a lenticular galaxy viewed edge-on. There is no evident spiral arm structure or significant dust lane absorption visible in this imaging, the color profile would imply the presence of an older stellar population or that it could be located in a relatively dense cluster environment. The estimated size indicates it is a relatively normal galaxy in the local universe. The overall impression is of a galaxy that is not actively forming stars at a high rate and doesn't appear to be undergoing any major mergers or significant tidal disturbances.
