The galaxy presents a generally smooth morphology, appearing largely featureless at this resolution. It exhibits a bright, concentrated central region that diminishes in intensity outwards. The overall shape is approximately round, with only slight deviations from a perfect circle. The galaxy's color profile suggests a dominant population of older stars, contributing to a yellow-reddish hue, particularly in the core. There is also a noticeable blue-green component, potentially indicating ongoing, but moderate, star formation in some regions. Evidence for major disturbances or ongoing mergers is not apparent, although subtle asymmetries may hint at minor gravitational interactions or internal dynamic processes. The size of the galaxy suggests it's a relatively large system.