The galaxy presents as a spiral type with a distinct disk structure. There are two very clearly defined spiral arms that emanate from a central bulge. The winding of these arms appears loose. The central bulge is of moderate size and exhibits a smooth texture with a yellowish hue. This suggests an older stellar population within the bulge. The overall color of the galaxy appears to be primarily in the green to redder end of the spectrum. While subtle, there seems to be evidence of possible recent or ongoing star formation within the spiral arms, though this is difficult to verify. The disk is presented nearly face-on relative to our line of sight, allowing a more complete visualization of its structure. There is no strong evidence of a significant bar structure. The overall shape does not suggest any major or minor ongoing merger events; the galaxy appears to be relatively undisturbed.
