The galaxy exhibits a generally smooth morphology, appearing largely featureless in this image. The central region displays a concentrated luminosity, potentially indicative of a significant bulge component. Color gradients are subtle, with a shift towards redder hues in the core and a slightly bluer tinge in the surrounding regions. This could suggest a relatively older stellar population dominating the central bulge, with ongoing or recent star formation in the outer areas. The overall rounded shape is consistent with an elliptical galaxy, though a weak disk component can't be entirely ruled out at this resolution. There might be indications of minor tidal disturbances, suggesting a possible past interaction or merger event, although this requires further investigation.
