This galaxy exhibits a smooth, elongated morphology, appearing as a flattened spheroid. The central region presents a concentrated luminosity gradient, suggesting a bulge component. The color profile indicates a dominant redder hue in the core, potentially indicative of an older stellar population, transitioning to slightly bluer tones in the outer regions, which may suggest more recent star formation activity. There is subtle evidence of minor disturbances or asymmetries in the outer regions. These disturbances could be due to interactions or mergers with smaller galaxies. The overall impression is that of a galaxy undergoing some level of morphological evolution. The smoothness of the light distribution suggests that this is not a pure spiral, but rather a late stage spiral or an elliptical galaxy.
