The galaxy exhibits a moderately elongated morphology, appearing somewhat cigar-shaped. It does not present a clear spiral structure or distinct disk component. The light distribution suggests a central bulge with a smoother, less defined structure. The galaxy displays color variations, transitioning from bluer hues in certain regions to redder tones elsewhere. There appears to be no strong indication of a major ongoing merger event. The galaxy does show indications of being a disturbed system, possibly from a previous minor merger or gravitational interactions. The estimated size of the galaxy indicates a substantial physical scale.
