The galaxy presents as a moderately bright, relatively compact object. Its overall morphology appears to be disc-dominated, though it lacks a clearly defined spiral structure in the available image. The central region shows a slight concentration of light, suggesting a bulge, but it is not highly pronounced. The galaxy exhibits a somewhat smooth texture, with only subtle hints of star-forming regions or dust lanes. The color profile suggests a mature stellar population, with a redder hue dominating, although some bluer regions exist. Based on its visual appearance, the galaxy likely has a moderate stellar mass. There are some indications of possible gravitational interactions, with subtle distortions in the galaxy's outer regions, which suggest that there could be a minor disturbance occurring. 
