The galaxy presents a predominantly smooth morphology, with a high degree of central concentration. The light profile suggests a lack of distinct spiral arm structure. The color appears relatively uniform across the galaxy, trending towards a redder hue, with some suggestion of yellower central area, which could be the core of the galaxy. The galaxy appears somewhat elliptical in shape, displaying a moderate degree of flattening, but it's close to round. There's no obvious evidence of major mergers or significant tidal disturbances. The relatively compact size suggests a correspondingly lower ongoing star formation rate.
