The galaxy presents a generally smooth morphology, appearing as an elongated, cigar-shaped structure. Little discernible internal structure is apparent. The light distribution suggests a relatively even stellar population throughout the galaxy, with a slight concentration towards the central region, though no distinct core or bulge is immediately obvious. The galaxy's color is generally red, hinting at an older stellar population and potentially lower ongoing star formation. There are no obvious signs of spiral arms or a prominent disk. There are no visible signs of active galactic nuclei activity or strong dust lanes. No significant interactions or disturbances are visible.