The galaxy appears as a moderately luminous object with an elliptical morphology. Its overall form seems relatively smooth, with no prominent spiral arm structures or significant dust lane obscuration visible. The light distribution suggests a centrally concentrated brightness profile, fading outwards from the core. There is a slight elongation, suggesting the galaxy is not perfectly spherical. The color index indicates a redder population of stars, potentially indicating an older stellar population and a lower rate of on-going star formation. The galaxy exhibits no signs of major mergers or significant tidal disturbances. It could be described as a red-sequence galaxy undergoing quiescent evolution.
