The galaxy presents a generally smooth and rounded morphology, suggestive of an elliptical galaxy. There is a high degree of central concentration, with the light intensity decreasing gradually from the core towards the edges. A minor asymmetry is present in the outer regions, possibly indicating a weak tidal interaction or past merger event. The color profile appears relatively uniform, with a redder hue dominating across the galaxy’s visible structure. No prominent spiral arms, dust lanes, or star-forming regions are immediately apparent.
