The galaxy presents as a relatively smooth, elliptical-like structure with a noticeable elongation. The central region exhibits a bright, concentrated luminosity, suggesting a significant stellar density or potentially an active galactic nucleus. The color profile transitions from a yellow-orange core to a bluer, less defined periphery, indicating a possible shift in stellar populations or dust content. The galaxy appears to be relatively isolated with no obvious signs of major mergers or tidal disturbances. However, there is a subtle asymmetry to the disk shape, which could be indicative of a past minor interaction. The overall morphology suggests a system that is evolving with a relatively low star formation rate.
