The galaxy presents an elliptical morphology, appearing as a largely smooth, centrally concentrated distribution of light. The core exhibits a yellowish hue, suggesting an older stellar population, potentially dominated by evolved stars. Moving outward from the core, the light appears to gradually fade, with a subtle transition towards bluer tones in the outer regions. This could indicate regions of more recent, but moderate, star formation. While largely smooth, there are some minor irregularities in the outer disk of the galaxy, perhaps indicating minor disturbances. The overall structure is elongated, exhibiting a non-circular shape without any clear indications of a dominant spiral arm structure. The light is centrally concentrated and not highly disturbed. Overall, this galaxy presents characteristics of a fairly massive galaxy with ongoing but not overwhelming star formation.
