The galaxy appears as a centrally concentrated, elliptical-like object. Its light profile seems relatively smooth, with no obvious spiral arm structures or prominent dust lanes visible. The galaxy's color is predominantly yellow, suggesting an older stellar population with a lower rate of ongoing star formation, supported by what appears to be a dearth of blue or distinctly red regions characteristic of young, massive stars or intense star-forming regions. The shape appears nearly circular. There are no obvious signs of major mergers or tidal disturbances, although some very slight asymmetry might indicate a minor interaction or internal dynamic process.
