The galaxy exhibits a generally smooth morphology with a slight central concentration of light. The color profile suggests a population of older stars, as indicated by the redder hues, implying a relatively low rate of current star formation activity. The galaxy appears mostly round in shape, with a notable absence of spiral arm structures or significant disk features. There may be a minor interaction or disturbance with another galaxy nearby. There is the suggestion of it merging or having merged with another galaxy. The overall appearance suggests a classification leaning toward elliptical or lenticular.
