The galaxy exhibits a generally smooth morphology with a subtle disk-like appearance, although it lacks prominent spiral arms. The central region shows a higher concentration of light, appearing more luminous and slightly redder in color, suggesting an older stellar population or dust obscuration. Moving outwards from the core, the galaxy becomes bluer, potentially indicating regions of ongoing or recent star formation. The galaxy's shape is elongated, displaying a notable deviation from perfect circularity. A slight disturbance or asymmetry is observed on one side of the galaxy, possibly hinting at a past or ongoing minor interaction with another galaxy, or internal activity. 
