The galaxy presents as a relatively smooth, disk-like structure, elongated along its major axis. The central region exhibits a concentrated, bright yellow-orange color, likely indicative of an older stellar population. Moving outwards from the core, the color transitions to a fainter, more diffuse blue-white, which suggests the presence of some younger, star-forming regions. While the overall structure appears largely undisturbed, a hint of asymmetry or possible minor disturbance can be observed in the outer regions of the disk, indicating a possible past or ongoing interaction. The galaxy's overall shape is somewhere between round and cigar shaped. The stellar mass of the galaxy is very high.
