The galaxy appears to be composed of a dominant, relatively smooth and concentrated central region, possibly a bulge. This bulge exhibits a yellowish hue, suggestive of an older stellar population. Extending from this central region is a fainter, somewhat elongated feature. The color of this feature appears bluer than the central bulge, possibly indicating a region of more recent star formation or a population of younger stars. Given the relative smoothness of the dominant bulge component, the galaxy leans towards an elliptical type, although the fainter, bluer extension hints at potential disk-like or irregular characteristics. There may be minor tidal features, but this requires further investigation to determine if this is a potential merger event or a more complex internal dynamic.
