The galaxy presents a generally smooth appearance with a notably elongated, cigar-like shape. A dominant central bulge exhibiting a yellowish hue is observed, suggesting a population of older stars. Faint blue tones are discernible near the edges of the galaxy, possibly indicative of younger stellar populations and ongoing star formation. There is no obvious indication of strong spiral arms or a well-defined disk. No major mergers are apparent, though a subtle asymmetry could suggest minor gravitational interactions or disturbances. The overall structure indicates a disk-dominated galaxy with no distinct core.
