The galaxy presents a generally smooth morphology, with a central bulge that appears largely featureless. The light is concentrated in the center and fades as you get further from the center. There is some presence of a disk structure. Its ellipticity suggests it is mostly round. No indications of active merging events or major disturbances are immediately apparent in the galaxy's morphology, though there is a hint of minor disturbance. The light from the galaxy has a redder hue. This could indicate an older stellar population or dust obscuration. The size is that of a massive galaxy. Overall, the galaxy appears to be a relatively evolved system, potentially transitioning towards a more passive state of star formation.
