The galaxy presents as an elongated, lenticular or cigar-shaped structure. It appears to possess a smooth, relatively featureless morphology, exhibiting a concentration of light towards the center. The central region of the galaxy displays a yellowish-orange hue, suggesting an older stellar population. Fainter blue tinges are observed at either end of the galaxy suggesting the presence of younger, hotter stars in those locations. No prominent spiral arms or significant dust lanes are readily discernible. The galaxy exhibits an overall undisturbed appearance with no significant signs of tidal disruption or interaction with neighboring galaxies. The dominant feature is the smoothness and the color gradient towards the center, hinting at a potentially evolved system with subdued star formation activity.
