The galaxy presents as a relatively smooth, centrally concentrated object. It has a roughly elliptical morphology, appearing more akin to a spheroid than a spiral. The color profile suggests an older stellar population, with a central yellowish hue fading outwards to redder tones. The relative lack of distinct features, such as spiral arms or prominent dust lanes, further supports a classification leaning toward an early-type galaxy. There might be a very faint disk component but it is hard to be sure. There is no apparent interaction or signs of a major merger. Based on morphology and color, the object appears to be an elliptical galaxy with suppressed star formation.