The galaxy presents as a slightly elongated, disk-like structure oriented roughly horizontally in the image. It exhibits a central bright region, possibly a bulge or a concentrated nucleus, with luminosity gradually decreasing outwards. The overall color is a mix of blue and white, suggesting a relatively high star formation rate and the presence of young, hot stars. There are hints of spiral arm structures, or at least an asymmetry to the light distribution, with one side appearing slightly more extended or disrupted. The outer edges are somewhat diffuse, without a sharp boundary, indicating a possible halo or ongoing interaction. Based on its intermediate color and smooth features, the galaxy appears to be in a transitional phase between a spiral and an elliptical galaxy, not actively forming a great many stars, but still having significant star formation. No clear signs of major mergers are visible, however the structure may be hinting at smaller interactions, or minor disturbances.
