The galaxy presents as a relatively smooth, elliptical form. Its color profile skews towards the redder end of the spectrum, indicating a likely older stellar population and a lower rate of on-going star formation. There is no visible spiral structure, bar, or evidence of significant dust lanes within this galaxy. Its overall shape is moderately rounded. There is no strong evidence of tidal disturbances or ongoing merger activity, suggesting it is a relatively settled and isolated system. The morphology appears dominated by an older, evolved stellar population.
