The galaxy presents as a moderately bright, relatively smooth object. Its morphology appears to be largely spheroidal, lacking any distinct spiral arm structure or prominent features indicative of a disk. The central region exhibits a concentrated, luminous core, suggesting a potentially significant stellar population density. The galaxy appears elliptical, with a minor axis that is slightly smaller than its major axis, classifying it as an elliptical galaxy. Color gradients across the galaxy are subtle, with a trend towards slightly redder hues concentrated towards the core. The outer regions show a gradual decline in surface brightness with no noticeable tidal features or interactions with neighboring galaxies. This object exhibits no signs of recent major merger events, although minor disturbances cannot be ruled out.
