The galaxy presents as a single, relatively smooth object with a concentrated central bulge. The light from the core appears reddish-orange, suggesting an older stellar population dominated by evolved stars. The overall shape is largely elliptical with some slight, subtle distortion. The outer regions of the galaxy display a greenish hue, potentially indicating the presence of some ongoing or recent star formation, although at a low rate. There is no evidence of prominent spiral arms or a well-defined disk structure. No signs of major mergers or tidal disturbances are visible. The galaxy appears to be isolated and undisturbed.
