The galaxy appears as a flattened spheroid, exhibiting a discernible disk-like structure. The central region presents a concentrated luminosity, indicative of a bulge or core component. There's a slight asymmetry in the overall shape, possibly hinting at a past or ongoing interaction or minor disturbance. The disk shows some indication of structure, but no clear spiral arm features are apparent. The color profile suggests a redder central region which is indicative of an older stellar population compared to the outer edges of the disk, which display bluer hues, potentially signifying younger, hotter stars and active star formation. The overall color suggests a relatively massive galaxy with moderate star formation activity. There's also a ring-like structure visible, possibly an area of increased star formation.
