The galaxy appears to be a relatively smooth, elliptical galaxy, exhibiting a concentrated central bulge. The color distribution suggests a population of older stars, giving it a yellowish to reddish hue. The galaxy shows signs of being somewhat spheroidal but is more likely in between spheroidal and cigar-shaped. There is little evidence of spiral arms or significant dust lanes. There are no signs of major disturbances within the galaxy that would suggest an ongoing major merger, but there could be some minor disturbances. The light is smoothly distributed, transitioning from a bright, saturated core to a more diffuse outer halo. The galaxy appears to be relatively isolated, showing no strong tidal interactions with neighboring galaxies in this image.
