The galaxy presents a generally smooth morphology, with a high degree of central concentration. The core region exhibits a yellowish-white hue, indicating a population of older stars. A slight extension of bluer light emanates from the periphery, suggestive of ongoing, albeit low, star formation. The overall shape approximates a slightly elongated spheroid, but is close to round. There is no strong visual evidence of spiral arm structure or a well-defined disk. Subtle disturbances cannot be completely ruled out based on this image.
