The galaxy appears to be a relatively smooth, elliptical type. There is minimal indication of spiral arm structure or significant dust lanes. The color profile suggests a population of stars with intermediate ages and a low rate of ongoing star formation. There is little evidence of recent major merger activity or significant tidal disturbances, although some minor irregularities cannot be ruled out. The light distribution appears centrally concentrated, indicating a well-established stellar population. The galaxy is moderately luminous. Based on color and morphology, the galaxy likely has a mass in the intermediate range.
