The galaxy presents a generally smooth morphology, appearing largely featureless in this image. Its overall shape is elliptical, showing a slight elongation but not a highly flattened disk. The central region exhibits a concentration of light, suggesting a bulge or core structure. Moving outward from the core, the light gradually diffuses, forming a halo. There is a slight blue-ish tint in some of the outer regions, possibly indicating some star formation. However, no prominent spiral arms or distinct dust lanes are discernible. There are no signs of significant tidal disturbances or ongoing merger activity. The galaxy appears to be relatively isolated in its environment, lacking nearby companions.
