The galaxy presents as an elongated, somewhat cigar-shaped structure. Its color profile suggests a higher concentration of older stellar populations, exhibiting a yellowish-red hue that is relatively uniform across the galactic body. There is no visually discernible spiral arm structure or dust lane obscuration. The galaxy lacks any obvious signs of active star formation regions based on the color profile, suggesting it is likely a passively evolving system. No significant morphological distortions or tidal features are visible, implying a relatively undisturbed evolutionary history. Overall, the galaxy appears to be an elliptical or lenticular galaxy viewed edge-on, characterized by a smooth light distribution and a lack of prominent star-forming regions.
