The galaxy appears to be a relatively smooth, centrally concentrated object. The light distribution suggests a dominant bulge component, potentially indicating an early-type galaxy morphology. There is some elongation, but it's more 'in between' round and cigar-shaped. Faint hints of asymmetric structure and possible tidal features are noticeable, suggesting potential past or ongoing minor interactions or disturbances. There is no clear presence of distinct spiral arms or a well-defined disk. There is some bluer light visible in the outer areas, indicating that there may be low levels of star formation occuring in the area, while the central bulge shows more red light. Overall, the galaxy appears as a mid-sized object undergoing some evolutionary process.
