The galaxy appears to be a large, luminous system with an overall smooth morphology. The light distribution suggests a roughly elliptical shape, exhibiting a moderately concentrated central bulge. There is some indication of disturbed morphology, with evidence suggesting a possible ongoing or recent merger event. This is seen in the irregular light distribution. The galaxy appears yellowish, suggesting an older stellar population with relatively little ongoing star formation. There is some faint blue light to the left, suggesting the presence of some younger stars or a region of more active star formation. Overall, the galaxy presents a complex and intriguing structure.
