The galaxy presents an elliptical morphology, with a smooth, featureless appearance. The light distribution is concentrated towards the center, fading gradually outward. The galaxy exhibits a yellowish-red hue, possibly indicative of an older stellar population and lower ongoing star formation rates. The shape is relatively smooth and in between that of a cigar shape and a perfect circle. There is no visible evidence of spiral arms or significant dust lanes. The galaxy appears to be relatively isolated, showing no obvious signs of tidal interaction or recent merger events. Based on the image, the galaxy is likely a massive system with a mature stellar population.
