This galaxy exhibits a somewhat elongated, cigar-like morphology. There is a notable concentration of light towards the central region, suggesting a bulge. The color appears to shift from a yellower hue in the core to a bluer tint at the edges. This may indicate a difference in stellar populations, with older, redder stars concentrated in the center and younger, bluer stars residing in the outer regions. The outer disk of the galaxy appears disturbed with features that might imply a minor interaction with a neighboring object or internal disturbances.
