The galaxy appears as a centrally concentrated, luminous object with an overall elliptical morphology. The light distribution is relatively smooth, exhibiting a lack of strong spiral arm structures or prominent dust lanes. The galaxy's color profile suggests a redder hue in comparison to typical spiral galaxies, potentially indicative of an older stellar population with a reduced rate of ongoing star formation. The galaxy's core presents a more intense concentration of light, which might indicate the presence of a supermassive black hole in the galactic nucleus. There are some irregularities present within the object; further study would be required to investigate whether it is minor disturbances from a past merger, or perhaps a statistical artifact. Overall, the galaxy exhibits characteristics consistent with a massive, evolved system.
