The galaxy appears to be an elliptical galaxy, exhibiting a generally smooth and featureless morphology. It has a moderate ellipticity, appearing elongated but not highly flattened, with a cigar shaped form. The central region presents a slightly brighter and more concentrated intensity profile, with the light gradually fading towards the edges of the galaxy. There is no discernible evidence of spiral arms, rings, or bar structures, suggesting a lack of significant ongoing star formation within a disk component. The color is more towards the red end of the spectrum, suggestive of an older stellar population dominated by red giant stars, however there are some components of blue light, which may suggest younger stars. There is no immediately obvious sign of any major interaction or merger event, but there is some minor disturbance.
