The galaxy presents an elliptical morphology, appearing relatively smooth and featureless in this observation. Its shape is somewhat elongated, exhibiting a cigar-like appearance. The light distribution suggests a concentration of older stars, giving it an overall yellowish-orange hue. There is no obvious indication of strong spiral arms or significant dust lanes. There does not appear to be any merging occurring with another galaxy, or evidence of a major disturbance. There is no indication of active star formation, suggesting it is potentially an older galaxy.