This galaxy appears to be a relatively smooth, elliptical system. It exhibits a pronounced cigar shape, indicating a deviation from perfect sphericity. The color profile suggests a primarily older stellar population, with a redder hue dominating the galaxy's overall appearance, but also hints at possibly some younger stars. There is no clear evidence of strong spiral arm structure or significant dust lanes. The galaxy does not present a disturbed morphology indicative of a recent major merger event. The light seems fairly concentrated.