The galaxy presents a predominantly smooth morphology, appearing as a single, centrally concentrated body. The color profile suggests a higher concentration of older stellar populations towards the center, indicated by the yellowish-orange hue. The outer regions exhibit a slight fading in intensity and transition toward redder tones. The galaxy displays an overall elliptical shape, though not perfectly spherical. There is some indication of minor disturbances in the structure, possibly suggestive of tidal interactions or past minor mergers. Although it appears as a single galaxy, there is evidence of a potential merger event, or at least some kind of interaction.
