The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a bright, concentrated core, indicating a high stellar density or potentially an active galactic nucleus. The light distribution appears symmetrical and centrally concentrated, diminishing gradually towards the outer regions. There is a notable absence of distinct spiral arms or prominent dust lanes. The color gradient is subtle, with a possibly bluer hue toward the center, suggesting the presence of younger stellar populations. Overall, the galaxy appears to be a well-formed, mature system with minimal signs of recent major disturbances or mergers.
