The galaxy presents as an elliptical-like system, exhibiting a concentrated central bulge that appears yellowish in color, potentially indicating an older stellar population. A flattened disk is also visible, oriented at a near edge-on angle relative to our line of sight. This disk shows some evidence of spiral structure, though it appears somewhat disrupted. The overall color of the disk shifts towards bluer hues further from the center, suggestive of ongoing star formation. There is an indication of some tidal disturbances or interactions, with asymmetric light distribution and morphological distortions. The galaxy appears to be relatively large and luminous.
