The galaxy presents as a moderately sized, elongated structure with a generally smooth appearance. It is characterized by a concentrated central bulge exhibiting a yellowish hue, which gradually fades into a slightly bluer disk-like structure. The central bulge appears relatively uniform in color and brightness, suggesting an older stellar population. There is little evidence of well-defined spiral arms; instead, the galaxy appears largely featureless. The color gradients across the structure suggest differential stellar populations. A slight warp or minor disturbance is visible on one side of the galaxy. The overall structure implies a galaxy undergoing either a late-stage merger or tidal disruption with no active star forming regions easily discernible in the image.
