This galaxy exhibits a roughly elliptical morphology, with a bright, concentrated central bulge region appearing almost stellar in its intensity. Surrounding the central bulge is a more diffuse halo, with colors indicating a mixture of stellar populations, including regions with bluer light indicative of younger stars, and redder regions suggestive of older populations. The galaxy does not appear to possess well-defined spiral arms or a prominent disk structure. Instead, it shows subtle features that could be interpreted as faint irregularities or tidal disturbances, potentially indicating past or ongoing minor interactions with other galaxies. There is also the possibility that the galaxy shows faint signs of merger activity. Overall, the galaxy appears as a system with a relatively smooth profile, but closer inspection reveals evidence of more complex evolutionary history.
