The galaxy presents as a spiral galaxy, observed at an oblique angle, exhibiting a moderate redshift. The central bulge appears bright and yellowish, suggesting an older stellar population likely dominated by red giant stars. A faint, disklike structure extends outwards from the bulge. The disk appears somewhat clumpy, hinting at regions of ongoing star formation. The arm structure is not well-defined, potentially indicating a galaxy that is either relatively undisturbed or has experienced some past interactions that have disrupted its spiral arms. There is also a faint amount of tidal disturbance observed, suggesting this galaxy might be merging with a smaller galaxy. The overall appearance suggests a galaxy with a mix of stellar populations and an ongoing evolutionary history. 
