The galaxy presents as a somewhat smooth, elliptical structure with a concentrated central bulge. There is evidence of a potential interaction or merger event occurring. Faint tidal features can be discerned extending from the main body of the galaxy. These features exhibit a disturbed morphology, suggesting gravitational interactions with another object, possibly a smaller satellite galaxy, or potentially an earlier merger stage. There appears to be evidence of star formation occurring within the galaxy, concentrated in certain regions, possibly induced by the interaction. The galaxy exhibits a relatively uniform color profile, with a dominant yellowish hue, suggesting an older stellar population.
