The galaxy presents a primarily smooth morphology. It is concentrated with a bright central bulge. The overall shape tends toward round, though slightly elongated. There is a hint of disklike structure, although it is not well defined. No significant tidal features or evidence of a major merger event are apparent. A subtle blue tint is visible in the disk, suggestive of ongoing star formation, although it appears subdued, with relatively low star formation rates. The redder central regions indicate an older stellar population.
