The galaxy appears as a single, relatively smooth object. There is a central bright, concentrated region, likely a bulge or core. The galaxy exhibits an overall elliptical or spheroidal shape. The color gradient suggests a population of evolved stars, with a slightly redder hue dominating the light. There is no apparent spiral structure or significant dust lanes visible, though a very faint disk may be present. There may be some very slight signs of minor gravitational disturbance. The galaxy exhibits an absolute magnitude that indicates it is a rather bright, and thus relatively large galaxy. The estimated size is less than 10 kpc which is fairly typical. The estimated stellar mass and star formation rate suggest this galaxy could be experiencing mild star formation.
