The galaxy presents a generally smooth morphology, lacking prominent spiral arms or a distinct bar structure. The overall shape is elongated, appearing somewhat cigar-shaped, and the light distribution suggests an elliptical-like structure. The central region displays a higher concentration of light, potentially indicating a galactic nucleus or a bulge. Color gradients are subtle but present, with the core appearing slightly more yellow/white compared to the outer regions which exhibit a faint blue hue. This could be indicative of an older stellar population in the core versus some ongoing star formation in the outer regions. No signs of major tidal disturbances or ongoing mergers are immediately apparent, although there might be evidence of minor disturbance in the outer part of the galaxy. 
