The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated, luminous core. There is a noticeable elongation, deviating from a perfectly circular morphology. The light distribution suggests a gradual decrease in luminosity outward from the central region, lacking distinct spiral arm features. Some minor distortions, possibly tidal features, may be present in the outskirts but are not highly prominent. The color profile appears relatively uniform, with a slightly redder hue, suggesting an older stellar population and less active star formation, although some star formation is still evident in the blue light.
