The galaxy presents as a moderately luminous, relatively smooth object. It displays an overall elliptical morphology, with a slightly elongated shape. The core region exhibits a concentrated, yellowish-white hue, suggesting a population of older stars. Surrounding the core is a fainter, bluer halo that is likely a mix of intermediate aged stars and some younger stars with relatively low star formation. There is no clear evidence of spiral arms, significant dust lanes, or a central bar structure, indicating a generally featureless disk. Minor disturbances may be present, though there is nothing to indicate a major merger event. The galaxy is fairly compact.
