The galaxy presents as a generally smooth object, exhibiting an elliptical morphology. It is highly concentrated, with a centrally brightened region indicative of a possible galactic nucleus or bulge. The light distribution is consistent with an E type galaxy. There is a very slight color gradient with the central regions being more yellow/red and the outer regions appearing slightly bluer. This might indicate the presence of older stellar populations in the center with some recent star formation in the outer regions. There is no obvious disk component, spiral arms, or bar structure visible. The galaxy appears relatively isolated, without significant signs of tidal interactions or ongoing mergers.
