The galaxy presents as a single, relatively smooth object with a concentrated central region. The color profile suggests a dominant population of older stars, indicated by the yellowish-orange hue. There is little evidence of spiral arms or significant dust lanes, suggesting it is either an elliptical galaxy or a face-on spiral with a low star formation rate. The light distribution appears symmetrical and centrally concentrated. There is no indication of a recent major merger, although minor disturbances can't be ruled out at this resolution. It appears round in shape and does not appear to be highly elongated or a cigar shape.
