This galaxy presents as a lenticular or possibly an elliptical system, exhibiting a generally smooth, diffuse morphology with little evidence of prominent spiral arms or distinct star-forming regions. The light distribution suggests a centrally concentrated structure, with a gradual decrease in luminosity towards the outer edges. The galaxy appears elongated, indicating a non-spherical shape. Color gradients are subtle, with a slightly redder hue in the central regions, potentially indicating an older stellar population and lower levels of on-going star formation. There might be a slight indication of tidal disturbances; further analysis would be necessary to confirm.
