The galaxy presents as an elliptical morphology, exhibiting a generally smooth appearance with little to no discernible substructure. The central region displays a high degree of luminosity, suggesting a concentrated stellar population or active galactic nucleus. Progressing outward from the core, the luminosity gradually diminishes. There may be a very subtle disk component. Overall, the galaxy appears relatively undisturbed, with no obvious signs of recent mergers or tidal interactions with other galaxies. The galaxy exhibits a color gradient, transitioning from a bluer hue in the central regions to a redder color towards the outer edges.
