The galaxy presents a generally smooth morphology, appearing largely featureless in this image. It exhibits a slightly elongated shape, but is mostly round. A central bulge region displays a bright, concentrated luminosity. The galaxy appears to be undergoing some sort of interaction, potentially a merger, which might be the cause of the slight elongation in an otherwise smooth galaxy. The overall color profile seems to indicate a dominance of older stellar populations, consistent with a relatively low rate of star formation.
