The galaxy presents an overall elliptical morphology, exhibiting a smooth light distribution without prominent spiral arms or a well-defined disk structure. The color gradient suggests a slightly redder core region, potentially indicating an older stellar population concentrated towards the galactic center. The outer regions show a bluer hue, hinting at the presence of some younger stars or ongoing, albeit subdued, star formation. There appears to be only a minor disturbance, suggesting that the system is not strongly interacting with other galaxies. It displays an intermediate ellipticity, leaning towards a more spheroidal rather than cigar-like shape.
