The galaxy presents an overall elliptical morphology, appearing somewhat elongated in shape. The central region exhibits a high degree of luminosity, indicating a concentrated stellar population and possibly an active galactic nucleus. Moving outward from the core, the luminosity gradually decreases. A noticeable feature is an irregular distribution of color across the galaxy. Patches of redder hues are visible in at least one of the outer regions, suggesting areas of older stellar populations or dust obscuration. The bluer colors suggests younger, hotter stars are forming, though not in significant amounts. There appears to be some disturbance to the smooth shape of the galaxy; perhaps an ongoing interaction with another galaxy or the result of a past merger event. There is no distinct spiral arm structure.
