The galaxy presents an elongated, cigar-shaped morphology. Its light profile suggests a relatively smooth distribution, with a brighter, condensed central region. This area could indicate a galactic bulge. The outer regions of the galaxy appear fainter and less defined, displaying a subtle blue hue. The overall structure suggests a system undergoing limited star formation activity, yet possessing a considerable stellar mass. There appears to be a minor gravitational disturbance; a slight asymmetry is present, possibly due to a recent or ongoing interaction.
