The galaxy appears to be a relatively smooth, elliptical galaxy with a concentrated central bulge. The light distribution suggests a high degree of spherical symmetry. There is a lack of any discernible spiral arm structure or dust lanes. The galaxy exhibits a yellowish-white color, indicating a stellar population dominated by older, less massive stars, and suggesting a quiescent or passively evolving system with reduced on-going star formation. No signs of significant tidal disturbances or mergers are immediately apparent, though the presence of minor disturbances cannot be ruled out at this resolution. The galaxy seems to be relatively isolated.
