The galaxy presents as a relatively smooth, elliptical-like structure. Its central region exhibits a concentrated, bright core, with luminosity decreasing gradually outward. The overall shape is elongated, appearing more like a flattened spheroid than a perfect circle, possibly exhibiting a subtle disk-like component. There appears to be a minor disturbance in the light distribution. The galaxy is transitioning from a disky galaxy to an elliptical one. It does not display any obvious spiral arms or significant dust lanes. The galaxy has a reddish hue throughout its extent, which could be indicative of an older stellar population and relatively low ongoing star formation.
