This galaxy appears to be a relatively smooth, elliptical galaxy. Its light profile suggests a high degree of sphericity, with no discernible spiral arms or bar structure. The central region exhibits a concentrated, bright core, indicative of a substantial bulge component. There is little evidence of significant dust lanes or active star formation regions within the visible spectrum. Its overall color is slightly redder than average, suggesting an older stellar population. Weak tidal features may be present, but are not obvious within this image. There is no evidence of any signs of recent or ongoing major mergers.
