The galaxy presents a generally smooth, rounded morphology. The light profile appears relatively concentrated towards the center, indicating a prominent bulge. The galaxy exhibits a colour gradient, transitioning from a bluer hue in what appears to be its central region to redder tones towards the outer edges. There is a very slight hint of a disk-like structure, although it is not well-defined. No obvious spiral arms or strong tidal features are discernible. The galaxy does not appear to be undergoing a major merger event, though a subtle asymmetry could suggest minor gravitational interactions. Given the colour profile and morphology, star formation is likely suppressed with the majority of the population consisting of older stars.
