The galaxy appears as a single object with a fairly round morphology, but with subtle hints of irregularities. While appearing largely smooth, closer inspection reveals a faint, potential disk-like structure or feature embedded within the galaxy. There are no obvious signs of a spiral arm structure, but a possible indication of minor disturbance or interaction is suggested by subtle asymmetry in the outer regions. The central region appears slightly brighter and more concentrated. The overall color profile indicates a relatively red population of stars or a significant presence of dust obscuring bluer light. There is no evidence of an ongoing merger event.
