The galaxy presents a distinctly elongated, cigar-shaped morphology. It appears largely smooth, with a bright, concentrated central bulge that dominates its luminosity profile. There is a hint of a disk, perhaps tightly wound, contributing to the observed flattening. Color gradients suggest an older stellar population, with the yellowish hue of the bulge indicative of evolved stars. Fainter blue hues are present in the outer regions, potentially signaling ongoing, albeit low, star formation. The overall structure suggests that it is unlikely this galaxy is undergoing any major mergers or strong tidal interactions. Some minor disturbance may be present.
