The galaxy presents a generally smooth morphology. Its shape is significantly elongated, resembling a cigar, with a high degree of axial ratio. A central bulge appears prominent, with a somewhat diffuse, extended disk. The color profile is observed to have a gradient, transitioning from bluer hues toward the outer regions, suggesting ongoing star formation. There appears to be no significant indication of major mergers or interactions. A slight irregularity can be seen, possibly indicating a minor disturbance.
