The galaxy presents a generally smooth morphology, appearing as an elliptical form. There is a slight elongation to its shape, deviating somewhat from a perfectly circular profile. The color gradient is relatively subtle across the galaxy's body, with a slightly bluer hue at one end, suggesting possible regions of more active star formation within the galaxy. A subtle disturbance is present in the galaxy's structure, indicating a minor gravitational interaction or past merger event. The galaxy’s overall luminosity suggests a significant stellar mass.
