The observed galaxy appears to be a relatively smooth, elliptical galaxy. Its morphology is largely featureless, lacking any prominent spiral arms or a well-defined disk structure. The galaxy exhibits a generally round shape, with no significant elongation or asymmetry evident. There is no indication of tidal tails, bridges, or other obvious signs of a recent or ongoing major merger event. There might be evidence of a minor disturbance within the galaxy. The galaxy's color indices suggest a relatively evolved stellar population, potentially comprised of older, redder stars, although precise age and metallicity determinations require spectroscopic analysis. Due to the apparent lack of visible dust lanes or HII regions, star formation may be minimal or absent.
