The galaxy presents an overall elliptical morphology. Its central region exhibits a high concentration of light, appearing bright and yellowish. Extending outwards from the core, there are hints of a more diffuse and disk-like structure, displaying a faint bluish hue. This suggests the presence of both older stellar populations in the central bulge and younger, star-forming regions within the outer disk. There is a slight asymmetry to the galaxy's structure, potentially indicating a past or ongoing interaction with another galaxy, as a slight disturbance is visible. Overall, the galaxy appears to be in a relatively evolved state with active star formation.
