The galaxy presents an elliptical morphology. Its core region exhibits a bright, concentrated luminosity, transitioning into a fainter, diffuse halo. Within the core, there appears to be a subtle, disklike structure oriented nearly edge-on with a distinct yellow color. This is surrounded by what appears to be a larger, less concentrated halo region, potentially indicating a transition zone or outer disk component. The overall color profile shifts from a relatively redder core to a bluer extended halo. There are some indications of minor disturbances, which could be due to tidal interactions with other galaxies. Overall, the galaxy presents an interesting case for further investigation into its formation history and dynamical interactions.
