The galaxy presents an overall elliptical morphology. Its light profile appears smooth and centrally concentrated. There is no obvious spiral arm structure or distinct features. The shape of the galaxy is more ovoid, leaning toward an "in-between" roundness, without being significantly elongated. There is no visible evidence of a major or minor merging event, nor a major disturbance in the overall structure. The central region appears slightly brighter and denser than the outer regions. The galaxy exhibits a color gradient, shifting from a slightly bluer hue in the inner regions to a redder hue in the outer regions. The galaxy displays an intermediate luminosity. The object's apparent size on the image suggests it is moderately distant. Its estimated stellar mass is within the average range for galaxies of this type. The rate of star formation within the galaxy is estimated to be low, which is consistent with an elliptical galaxy exhibiting older stellar populations and minimal ongoing star formation.
