The galaxy presents as a somewhat smooth, disk-shaped structure, elongated in appearance, suggesting an elliptical morphology or a spiral galaxy viewed at an angle. The central region exhibits a concentrated, bright core with a yellowish-white hue, possibly indicative of an older stellar population. Moving outwards from the core, the disk shows a gradual fading of luminosity. Subtle color variations are present in the outer regions of the disk, with hints of bluer tones intermixed with reddish hues, potentially indicating regions of active star formation alongside older stellar populations. There are no obvious signs of strong disturbances or major mergers, although there seems to be a small irregularity in the disk that suggests a minor interaction. 
