The galaxy presents an elongated, cigar-shaped morphology. It appears largely smooth in texture, with a bright central bulge that graduates outwards. There is a possible presence of a disk component. The color profile suggests a dominance of older stellar populations, with a yellowish-red hue. There is a slight hint of blue near one edge of the disk, suggesting a small amount of recent star formation. No significant tidal features or indications of major mergers are apparent, though minor disturbances cannot be ruled out. Overall, the galaxy appears to be a relatively isolated system that is well past its peak of star formation.
