The galaxy exhibits a morphology that is neither purely elliptical nor a well-defined spiral. It appears to be a disk galaxy with a bulge, but it also has a disturbed appearance, possibly due to interactions. There appears to be an amorphous shape with a bright, concentrated central region exhibiting a yellowish hue, suggesting an older stellar population. Surrounding the core, there's a more diffuse, bluish glow indicative of younger, hotter stars and active star formation. The galaxy doesn't have a clear spiral arm structure but shows hints of disturbed arms or tidal features that extend out into space. There is also potential evidence of merging or interaction.
