The observed galaxy presents an overall elliptical morphology, appearing cigar-shaped with a high degree of central concentration. Its light profile is smooth, lacking prominent spiral arm structures or other distinct features. The galaxy's core exhibits a bright, concentrated emission, suggestive of an older stellar population, potentially with a contribution from a central supermassive black hole's active galactic nucleus. Color gradients are subtle, but it shows a slightly bluer hue towards its outer regions, possibly indicating the presence of some younger stars or ongoing, albeit minimal, star formation in the periphery. The galaxy lacks any obvious signs of recent major mergers or tidal disturbances, retaining a regular and undisturbed structure.
