The galaxy appears to be an elliptical galaxy, showing a largely featureless, smooth structure without prominent spiral arms or a defined disk. It has a somewhat elongated shape, appearing more like a flattened spheroid than a perfect sphere. There are no obvious signs of a major ongoing merger, though a slight asymmetry might indicate minor tidal interactions or disturbances. The galaxy displays a relatively concentrated central region that decreases in luminosity toward its outer edges. The color profile suggests a population of older stars, as the galaxy emits strongly in the redder wavelengths. There appears to be some low-level activity at the edges of the galaxy, possibly in the form of disrupted star clusters or faint star formation.
