The galaxy presents a predominantly smooth morphology, appearing largely featureless in this observation. Its overall shape tends toward elliptical, displaying a moderate ellipticity, with an intermediate form between perfectly round and elongated. There is no strong visual evidence of spiral arms, bars, or other distinct structures commonly found in disk galaxies. The galaxy's central region exhibits a bright, concentrated core, suggesting the presence of a significant stellar population density, potentially harboring a supermassive black hole. A more diffuse halo of light surrounds the central core, gradually fading into the background sky. While the galaxy exhibits a relatively smooth appearance, there might be some subtle signs of minor disturbance present but does not appear to be in a major merger. The color profile exhibits a gradient, transitioning from redder hues in the central regions to slightly bluer tones in the outer halo. Overall, the galaxy appears to be a relatively massive and evolved system.
