The galaxy presents as a relatively smooth, rounded structure with a concentrated central region. Its color is predominantly yellow, suggesting an older stellar population with fewer young, hot stars. There's a subtle color gradient from the core outwards, perhaps indicating a radial variation in stellar age or metallicity. There appears to be a slight asymmetry in the outer regions, potentially indicative of past minor interactions. The overall morphology appears quiescent, lacking prominent spiral arms or significant dust lanes. The galaxy appears to be a relatively massive system. The star formation rate seems to be quite low.
