The galaxy presents an elliptical morphology, exhibiting a relatively smooth and concentrated light distribution. The central region appears bright and somewhat unresolved, suggesting a significant stellar density or perhaps an active galactic nucleus. Progressing outwards from the center, the light gradually diminishes, forming a diffuse halo that extends to a considerable distance. There is a subtle color gradient evident, transitioning from a yellowish-white core to slightly bluer hues in the outer regions. While the galaxy appears primarily smooth, there are hints of minor irregularities or faint, diffuse features within the halo, possibly indicative of past minor merger events or ongoing star formation. Overall, the galaxy appears to be a massive system, with significant luminosity and extent.
