The galaxy presents as a moderately faint, elongated lenticular type with a central, brighter core region indicating a concentration of older stellar populations. The primary color is a soft white-blue, suggesting a mix of young, hot stars and an underlying population of older, cooler stars. The overall structure appears largely smooth with some faint hints of disk-like features, but no distinct spiral arms are discernible. There appears to be only minor disturbances in the structure, indicating it is not currently undergoing a major merger event. The galaxy's elongated shape suggests it is viewed at an oblique angle.