The galaxy presents as a slightly elongated structure, with a dominant central bulge that appears relatively smooth. The galaxy's overall color is a yellowish-white, suggesting an older stellar population. There is an indication of a faint, dusty disk component, with subtle hints of spiral arm structure, although these are not sharply defined. One end of the galaxy seems brighter and more distinct. The galaxy does not appear to be undergoing any major mergers, although there is an object nearby that could be a satellite galaxy or experiencing a minor disturbance with the main galaxy. There is a slight asymmetry to the galaxy's overall shape, perhaps due to interactions or internal dynamics.
