The galaxy presents a generally smooth morphology, appearing largely elliptical in shape with a high degree of central concentration. The core region is bright, suggesting a significant density of stars. There is a slight elongation observed, but the galaxy is largely rounded, showing no prominent disk structure. The color profile is dominated by warmer, redder tones throughout, indicative of an older stellar population with relatively little ongoing star formation. There is a possible minor disturbance present, which is likely a merging event with another galaxy. The size and shape measurements indicate it is a typical galaxy in terms of size.
