The galaxy presents as a diffuse, oblong structure. Its overall color is a muted white, with a slightly brighter, more concentrated central region. This suggests a concentration of older stellar populations and potentially a supermassive black hole at the galactic center. The outer regions exhibit a faint bluish tinge, possibly indicating the presence of some younger, hotter stars, although not in significant numbers. The morphology hints at a spiral or disk galaxy viewed at an oblique angle, but the resolution is insufficient to definitively confirm spiral arm structures. There may be some signs of a minor disturbance in the lower left side of the galaxy. Based on its red color, modest absolute magnitude, and inferred stellar mass, it is likely a relatively quiescent galaxy with a low star formation rate. The galaxy appears to be largely isolated, with no obvious signs of recent or ongoing major merger activity.
