The galaxy presents with a moderately bright core, exhibiting a predominantly blue-green hue. This suggests a significant population of young, hot stars and active star formation. The morphology appears to be primarily disk-like, oriented approximately horizontally across the frame. Faint extensions are visible on either side of the central bulge, indicating the presence of a disk structure. There appears to be a slight irregularity or disturbance in the disk, hinting at a possible minor merger or tidal interaction. Overall, the galaxy is a well-defined but not perfectly symmetrical system, characterized by a mix of features indicative of ongoing stellar activity and potential past interactions.
