The galaxy presents as a largely homogenous elliptical structure with a high degree of central concentration. The overall color appears to be dominated by light in the redder portions of the spectrum, suggesting an older stellar population. There is little evidence of spiral arm structures or significant dust lanes. The object appears to have a smooth profile, lacking the distinct irregularities that would indicate a recent merger event or active star formation regions. Some minor asymmetry may be present in the outskirts of the galaxy. The galaxy appears to be relatively isolated in this field, with no obvious companion galaxies nearby, and no tidal distortion is apparent.
