The galaxy appears to be a luminous elliptical galaxy, exhibiting a smooth, largely featureless morphology. It presents as a concentrated spheroid with a high degree of central concentration. The color profile suggests an older stellar population, with a yellow to reddish hue indicating a relative lack of ongoing star formation. There is no obvious disk component or spiral arm structure visible. The galaxy appears roughly circular, with only a slight deviation from perfect roundness. No significant tidal disturbances or interactions with nearby galaxies are readily apparent, suggesting a relatively isolated system.
